cxprep/chandra.txt: prepare 2012 images for registration
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Peter Williams
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@ -6,11 +6,10 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-499.jpg
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astropix_ids: chandra|499
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credits> X-ray: NASA/CXC/Rutgers/J.Hughes; This galaxy cluster, which has been
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nicknamed "El Gordo" for the "big" or "fat" one in Spanish, is a remarkable
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object. Found i...
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credits> X-ray: NASA/CXC/Rutgers/J.Hughes et al, Optical: ESO/VLT/Pontificia
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Universidad. Catolica de Chile/L.Infante & SOAR
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(MSU/NOAO/UNC/CNPq-Brazil)/Rutgers/F.Menanteau, IR: NASA/JPL/Rutgers/F.Menanteau
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wip: yes
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---
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@scene
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@ -19,9 +18,12 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-499L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/elgordo/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-499.jpg
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text> El Gordo
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text> "El Gordo" is the nickname given to an extraordinary galaxy cluster in the
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distant universe. A composite image shows El Gordo in X-ray light from NASA's
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Chandra X-ray Observatory in blue, along with optical data from the European
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Southern Observatory's Very Large Telescope (VLT) in red, green, and blue, and
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infrared emission from the NASA's Spitzer Space Telescope in red and orange.
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wip: yes
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---
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@image
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@ -31,11 +33,8 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-500.jpg
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astropix_ids: chandra|500
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credits> X-ray: NASA/CXC/SAO/I.Lovchinsky; G350.1+0.3 is a young and
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exceptionally bright supernova remnant in our Galaxy. While many supernova
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remnants are nearly circul...
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credits> X-ray: NASA/CXC/SAO/I.Lovchinsky et al, IR: NASA/JPL-Caltech
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wip: yes
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---
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@scene
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@ -44,9 +43,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-500L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/g350/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-500.jpg
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text> G350.1-0.3
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text> Vital clues about the devastating ends to the lives of massive stars can
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be found by studying the aftermath of their explosions. Chandra's image of the
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supernova remnant known as G350.1-0.3 is an example of this important
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investigation. This stellar debris field is located some 14,700 light years from
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the Earth toward the center of the Milky Way. Evidence from Chandra and from
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ESA's XMM-Newton telescope suggest that a compact object within G350.1-0.3 may
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be the dense core of the star that exploded.
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wip: yes
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---
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@image
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@ -56,11 +60,8 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-501.jpg
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astropix_ids: chandra|501
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credits> X-ray: NASA/CXC/MIT/F. Baganoff ; A new study provides a possible
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explanation of mysterious X-ray flares detected by Chandra over the period of
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several years. It...
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credits> X-ray: NASA/CXC/MIT/F. Baganoff et al.; Illustrations: NASA/CXC/M.Weiss
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wip: yes
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---
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@scene
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@ -69,9 +70,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-501L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/sgra/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-501.jpg
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text> Sagittarius A*
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text> This image from NASA's Chandra X-ray Observatory shows the center of our
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Galaxy, with a supermassive black hole known as Sagittarius A* (Sgr A* for
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short) in the center. Using intermittent observations over several years,
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Chandra has detected X-ray flares about once a day from Sgr A*. An asteroid that
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undergoes a close encounter with another object, such as a star or planet, can
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be thrown into an orbit headed towards Sgr A*, as seen in a series of artist's
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illustrations beginning with the top-right panel.
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wip: yes
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---
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@image
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@ -81,11 +87,9 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-503.jpg
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astropix_ids: chandra|503
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credits> NASA, ESA, CFHT, CXO, M.J. Jee (; This composite image shows the
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distribution of dark matter, galaxies, and hot gas in the core of the merging
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galaxy cluster Abel...
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credits> NASA, ESA, CFHT, CXO, M.J. Jee (University of California, Davis), and
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A. Mahdavi (San Francisco State University)
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wip: yes
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---
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@scene
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@ -94,9 +98,11 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-503L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/a520/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-503.jpg
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text> Image File
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text> This composite image shows the distribution of dark matter, galaxies, and
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hot gas in the core of the merging galaxy cluster Abell 520, formed from a
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violent collision of massive galaxy clusters that is located about 2.4 billion
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light years from Earth.
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wip: yes
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---
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@image
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@ -106,11 +112,9 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-504.jpg
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astropix_ids: chandra|504
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credits> X-ray: NASA/CXC/Caltech/A.Newman; Two teams of astronomers have used
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data from Chandra and other telescopes to map the distribution of dark matter in
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three dimens...
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credits> X-ray: NASA/CXC/Caltech/A.Newman et al/Tel Aviv/A.Morandi &
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M.Limousin; Optical: NASA/STScI, ESO/VLT, SDSS
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wip: yes
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---
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@scene
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@ -119,9 +123,13 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-504L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/a383/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-504.jpg
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text> Abell 383
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text> Two teams of astronomers have used data from NASA's Chandra X-ray
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Observatory and other telescopes to map the distribution of dark matter in a
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galaxy cluster known as Abell 383, which is located about 2.3 billion light
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years from Earth. Not only were the researchers able to find where the dark
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matter lies in the two dimensions across the sky, they were also able to
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determine how the dark matter is distributed along the line of sight.
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wip: yes
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---
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@image
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@ -130,11 +138,8 @@ copyright: Public domain
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license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-505.jpg
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credits> Illustration: NASA/CXC/M.Weiss; ; This two-panel graphic compares an
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artist's illustration (left) of a simplified picture of the inner layers of a
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star just befor...
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credits> llustration: NASA/CXC/M.Weiss; X-ray: NASA/CXC/GSFC/U.Hwang & J.Laming
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wip: yes
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---
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@scene
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@ -143,9 +148,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-505L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/casa/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-505.jpg
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text> Image File
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text> A new X-ray study of the remains of an exploded star indicates that the
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supernova that disrupted the massive star may have turned it inside out in the
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process. Using very long observations of Cassiopeia A (or Cas A), a team of
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scientists has mapped the distribution of elements in the supernova remnant in
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unprecedented detail. This information shows where the different layers of the
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pre-supernova star are located three hundred years after the explosion, and
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provides insight into the nature of the supernova.
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wip: yes
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---
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@image
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@ -155,11 +165,8 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-506.jpg
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astropix_ids: chandra|506
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credits> X-ray: NASA/CXC/UCDavis/W.Dawson; This composite image shows Chandra
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(red) and Hubble (yellow and white) data of the galaxy cluster system that has
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been nicknamed...
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credits> X-ray: NASA/CXC/UCDavis/W.Dawson et al; Optical: NASA/STScI/UCDavis/W.Dawson et al.
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wip: yes
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---
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@scene
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@ -168,9 +175,12 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-506L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/musketball/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-506.jpg
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text> Image File
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text> Using a combination of powerful observatories in space and on the ground,
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astronomers have observed a violent collision between two galaxy clusters in
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which so-called normal matter has been wrenched apart from dark matter through a
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violent collision between two galaxy clusters. The newly discovered galaxy
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cluster is called DLSCL J0916.2+2951.
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wip: yes
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---
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@image
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@ -180,11 +190,9 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-507.jpg
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astropix_ids: chandra|507
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credits> X-ray: NASA/CXC/PSU/L.Townsley e; This composite of 30 Doradus, aka the
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Tarantula Nebula, contains data from Chandra (blue), Hubble (green), and Spitzer
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(red). L...
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credits> X-ray: NASA/CXC/PSU/L.Townsley et al.; Optical: NASA/STScI; Infrared:
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NASA/JPL/PSU/L.Townsley et al.
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wip: yes
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---
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@scene
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@ -193,9 +201,15 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-507L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/30dor/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-507.jpg
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text> Tarantula Nebula
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text> 30 Doradus is located in the neighboring galaxy called the Large
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Magellanic Cloud, and is one of the largest star-forming regions located close
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to the Milky Way. At the center of 30 Doradus, thousands of massive stars are
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blowing off material and producing intense radiation along with powerful winds.
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The Chandra X-ray Observatory detects gas that has been heated to millions of
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degrees by these stellar winds and also by supernova explosions. These X-rays,
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colored blue in this composite image, come from shock fronts — similar to sonic
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booms — formed by this high-energy stellar activity.
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wip: yes
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---
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@image
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@ -205,11 +219,8 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-511.jpg
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astropix_ids: chandra|511
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credits> X-ray: NASA/CXC/Royal Military C; This composite image shows the galaxy
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UGC 5189A in X-ray data from Chandra (purple) and optical data from Hubble (red,
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green and...
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credits> X-ray: NASA/CXC/Royal Military College of Canada/P.Chandra et al); Optical: NASA/STScI
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wip: yes
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---
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@scene
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@ -218,9 +229,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-511L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/sn2010/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-511.jpg
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text> SN 2010jl
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text> Observations with NASA's Chandra X-ray Observatory have provided X-ray
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evidence of a supernova shock wave breaking through a cocoon of gas surrounding
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the star that exploded. This discovery may help astronomers understand why some
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supernovas are much more powerful than others. On November 3, 2010, a supernova
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was discovered in the galaxy UGC 5189A, located about 160 million light years
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away. Supernove SN 2010jl is the very bright X-ray source near the top of the
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galaxy.
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wip: yes
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---
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@image
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@ -230,11 +246,8 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-512.jpg
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astropix_ids: chandra|512
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credits> NASA/JPL-Caltech/ESA/CfA; This composite image of M101 (aka, the
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"Pinwheel Galaxy") combines data from four of NASA's space-based telescopes.
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X-rays from...
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credits> X-ray: NASA/CXC/SAO; IR & UV: NASA/JPL-Caltech; Optical: NASA/STScI
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wip: yes
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---
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@scene
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@ -243,9 +256,11 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-512L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/m101/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-512.jpg
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text> M101
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text> This image of the Pinwheel Galaxy, or also known as M101, combines data in
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the infrared, visible, ultraviolet and X-rays from four of NASA's space-based
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telescopes. This multi-spectral view shows that both young and old stars are
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evenly distributed along M101's tightly-wound spiral arms.
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wip: yes
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---
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@image
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@ -255,11 +270,8 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-513.jpg
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astropix_ids: chandra|513
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credits> X-ray: NASA/CXC/SAO/F.Civano et ; Chandra and other telescopes have
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shown that the galaxy CID-42 likely contains a massive black hole being ejected
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at several mil...
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credits> X-ray: NASA/CXC/SAO/F.Civano et al; Optical: NASA/STScI; Optical (wide field): CFHT, NASA/STScI
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wip: yes
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---
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@scene
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@ -268,9 +280,16 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-513L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/cid42/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-513.jpg
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text> Image File
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text> The galaxy at the center of this image contains an X-ray source, CID-42,
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with exceptional properties. Researchers think that CID-42 contains a massive
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black hole being ejected from its host galaxy at several million miles per hour.
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The outlined box in the main image represents the more localized view of CID-42
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that is shown in the three separate boxes on the right-hand side of the image.
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At the top is an image from the Chandra X-ray Observatory. The X-ray emission is
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concentrated in a single source, corresponding to one of the two sources seen in
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deep observations by Hubble, which is shown in the middle inset box. The bottom
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inset shows how the X-rays align with the optical data in the two insets above.
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wip: yes
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---
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@image
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@ -280,11 +299,9 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-515.jpg
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astropix_ids: chandra|515
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credits> X-ray: NASA/CXC/UC Berkeley/J.To; Using Chandra, XMM-Newton, and the
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Parkes radio telescope, researchers have found evidence for what may be the
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fastest moving pu...
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credits> X-ray: NASA/CXC/UC Berkeley/J.Tomsick et al & ESA/XMM-Newton, Optical:
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DSS; IR: 2MASS/UMass/IPAC-Caltech/NASA/NSF
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wip: yes
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---
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@scene
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@ -293,9 +310,15 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-515L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/igrj11014/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-515.jpg
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text> IGR J11014-6103
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text> Researchers using three different telescopes — NASA's Chandra X-ray
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Observatory and ESA's XMM-Newton in space, and the Parkes radio telescope in
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Australia — may have found the fastest moving pulsar ever seen: IGR J1104-6103.
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The evidence for this potentially record-breaking speed comes, in part, from the
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features highlighted in this composite image. X-ray observations from Chandra
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(green) and XMM-Newton (purple) have been combined with infrared data from the
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2MASS project and optical data from the Digitized Sky Survey (colored red, green
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and blue, but appearing in the image as white).
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wip: yes
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---
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@image
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@ -305,11 +328,8 @@ license_id: CC-PDDC
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-518.jpg
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astropix_ids: chandra|518
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credits> X-ray: NASA/CXC/STScI/K.Long et ; Using Chandra, astronomers have
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detected X-rays from the remains of a supernova that was spotted from Earth over
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50 years ago. ...
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credits> X-ray: NASA/CXC/STScI/K.Long et al., Optical: NASA/STScI
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wip: yes
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---
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@scene
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@ -318,9 +338,17 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-518L{1}X{2}Y{3}.pn
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outgoing_url: https://chandra.harvard.edu/photo/2012/m83sn/
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thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-518.jpg
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text> M83
|
||||
text> Over fifty years ago, a supernova was discovered in M83, a spiral galaxy
|
||||
about 15 million light years from Earth. Astronomers have used NASA's Chandra
|
||||
X-ray Observatory to make the first detection of X-rays emitted by the debris
|
||||
from this explosion. Named SN 1957D because it was the fourth supernova to be
|
||||
discovered in the year of 1957, it is one of only a few located outside of the
|
||||
Milky Way galaxy that is detectable, in both radio and optical wavelengths,
|
||||
decades after its explosion was observed. In 1981, astronomers saw the remnant
|
||||
of the exploded star in radio waves, and then in 1987 they detected the remnant
|
||||
at optical wavelengths, years after the light from the explosion itself became
|
||||
undetectable.
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@image
|
||||
|
|
@ -329,11 +357,8 @@ copyright: Public domain
|
|||
license_id: CC-PDDC
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-519.jpg
|
||||
|
||||
credits> X-ray: NASA/CXC/MIT/M.McDonald;; The Phoenix Cluster is an
|
||||
extraordinary galaxy cluster that is breaking several important astronomical
|
||||
records. The composite i...
|
||||
credits> X-ray: NASA/CXC/MIT/M.McDonald; UV: NASA/JPL-Caltech/M.McDonald; Optical: AURA/NOAO/CTIO/MIT/M.McDonald; Illustration: NASA/CXC/M.Weiss
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@scene
|
||||
|
|
@ -342,9 +367,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-519L{1}X{2}Y{3}.pn
|
|||
outgoing_url: https://chandra.harvard.edu/photo/2012/phoenix/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-519.jpg
|
||||
|
||||
text> Phoenix Cluster
|
||||
text> The image on the left shows the newly discovered Phoenix Cluster, located
|
||||
about 5.7 billion light years from Earth. This composite includes an X-ray image
|
||||
from NASA's Chandra X-ray Observatory in purple, an optical image from the 4m
|
||||
Blanco telescope in red, green and blue, and an ultraviolet (UV) image from
|
||||
NASA's Galaxy Evolution Explorer (GALEX) in blue. The Chandra data show hot gas
|
||||
in the cluster and the optical and UV images show galaxies in the cluster and in
|
||||
nearby parts of the sky.
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@image
|
||||
|
|
@ -354,11 +384,8 @@ license_id: CC-PDDC
|
|||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-520.jpg
|
||||
astropix_ids: chandra|520
|
||||
|
||||
credits> X-ray: NASA/CXC/U.Mich./S.Oey, I; The star cluster NGC 1929 contains
|
||||
massive stars that produce intense radiation, expel matter at high speeds, and
|
||||
race through t...
|
||||
credits> X-ray: NASA/CXC/U.Mich./S.Oey, IR: NASA/JPL, Optical: ESO/WFI/2.2-m
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@scene
|
||||
|
|
@ -367,9 +394,13 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-520L{1}X{2}Y{3}.pn
|
|||
outgoing_url: https://chandra.harvard.edu/photo/2012/n1929/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-520.jpg
|
||||
|
||||
text> Image File
|
||||
text> This composite image shows a superbubble in the Large Magellanic Cloud
|
||||
(LMC), a small satellite galaxy of the Milky Way, located about 160,000 light
|
||||
years from Earth. Many new stars, some of them very massive, are forming in the
|
||||
star cluster NGC 1929, which is embedded in the nebula N44. The massive stars
|
||||
produce intense radiation, expel matter at high speeds, and race through their
|
||||
evolution to explode as supernovas.
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@image
|
||||
|
|
@ -379,11 +410,8 @@ license_id: CC-PDDC
|
|||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-521.jpg
|
||||
astropix_ids: chandra|521
|
||||
|
||||
credits> X-ray: NASA/CXC/SAO/D.Patnaude, ; This composite image of Kepler's
|
||||
supernova remnant shows different colors ranging from lower to higher energies:
|
||||
red, yellow, gr...
|
||||
credits> X-ray: NASA/CXC/SAO/D.Patnaude, Optical: DSS
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@scene
|
||||
|
|
@ -392,9 +420,16 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-521L{1}X{2}Y{3}.pn
|
|||
outgoing_url: https://chandra.harvard.edu/photo/2012/kepler/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-521.jpg
|
||||
|
||||
text> Kepler's Supernova Remnant
|
||||
text> In 1604, a new star appeared in the night sky that was much brighter than
|
||||
Jupiter and dimmed over several weeks. This event was witnessed by sky watchers
|
||||
including the famous astronomer Johannes Kepler. Centuries later, the debris
|
||||
from this exploded star is known as the Kepler supernova remnant. Astronomers
|
||||
have long studied the Kepler supernova remnant and tried to determine exactly
|
||||
what happened when the star exploded to create it. New analysis of a long
|
||||
observation from NASA's Chandra X-ray Observatory is providing more clues. This
|
||||
analysis suggests that the supernova explosion was not only more powerful, but
|
||||
might have also occurred at a greater distance, than previously thought.
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@image
|
||||
|
|
@ -404,11 +439,8 @@ license_id: CC-PDDC
|
|||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-524.jpg
|
||||
astropix_ids: chandra|524
|
||||
|
||||
credits> X-ray: NASA/CXC/George Mason Uni; One of the lowest mass supermassive
|
||||
black holes ever observed in the middle of a galaxy has been identified, thanks
|
||||
to NASA's Ch...
|
||||
credits> X-ray: NASA/CXC/George Mason Univ/N.Secrest et al; Optical: SDSS
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@scene
|
||||
|
|
@ -417,9 +449,12 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-524L{1}X{2}Y{3}.pn
|
|||
outgoing_url: https://chandra.harvard.edu/photo/2012/ngc4178/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-524.jpg
|
||||
|
||||
text> NGC 4178
|
||||
text> One of the lowest mass supermassive black holes ever observed in the
|
||||
middle of a galaxy has been identified, thanks to NASA's Chandra X-ray
|
||||
Observatory and several other observatories. The host galaxy is of a type not
|
||||
expected to harbor supermassive black holes, suggesting that this black hole,
|
||||
while related to its supermassive cousins, may have a different origin.
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@image
|
||||
|
|
@ -429,11 +464,8 @@ license_id: CC-PDDC
|
|||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-525.jpg
|
||||
astropix_ids: chandra|525
|
||||
|
||||
credits> X-ray: NASA/CXC/SAO/J.Drake et a; This composite image of the star
|
||||
cluster Cygnus OB2 contains X-rays from Chandra (blue), infrared data from
|
||||
Spitzer (red), and o...
|
||||
credits> X-ray: NASA/CXC/SAO/J.Drake et al, Optical: Univ. of Hertfordshire/INT/IPHAS, Infrared: NASA/JPL-Caltech
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@scene
|
||||
|
|
@ -442,9 +474,16 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-525L{1}X{2}Y{3}.pn
|
|||
outgoing_url: https://chandra.harvard.edu/photo/2012/cygob2/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-525.jpg
|
||||
|
||||
text> Cygnus OB2
|
||||
text> The Milky Way and other galaxies in the universe harbor many young star
|
||||
clusters and associations that each contain hundreds to thousands of hot,
|
||||
massive, young stars known as O and B stars. The star cluster Cygnus OB2
|
||||
contains more than 60 O-type stars and about a thousand B-type stars. At a
|
||||
relatively nearby distance to Earth of about 5,000 light years, Cygnus OB2 is
|
||||
the closest massive cluster. Deep observations with NASA's Chandra X-ray
|
||||
Observatory of Cygnus OB2 have been used to detect the X-ray emission from the
|
||||
hot outer atmospheres, or coronas, of young stars in the cluster and to probe
|
||||
how these great star factories form and evolve.
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@image
|
||||
|
|
@ -454,11 +493,8 @@ license_id: CC-PDDC
|
|||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-526.jpg
|
||||
astropix_ids: chandra|526
|
||||
|
||||
credits> Inset X-ray (NASA/CXC/IAA-CSIC/M; The inset image on the right is a
|
||||
close-up view of A30 showing X-ray data from NASA's Chandra X-ray Observatory in
|
||||
purple and Hu...
|
||||
credits> Inset X-ray (NASA/CXC/IAA-CSIC/M.Guerrero et al); Inset Optical (NASA/STScI); Widefield X-ray (ESA/XMM-Newton); Widefield Optical (NSF/NOAO/KPNO)
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@scene
|
||||
|
|
@ -467,9 +503,16 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-526L{1}X{2}Y{3}.pn
|
|||
outgoing_url: https://chandra.harvard.edu/photo/2012/a30/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-526.jpg
|
||||
|
||||
text> Abell 30
|
||||
text> These images of the planetary nebula Abell 30, (a.k.a. A30), show one of
|
||||
the clearest views ever obtained of a special phase of evolution for these
|
||||
objects. The inset is a close-up view of A30 showing X-ray data from NASA's
|
||||
Chandra X-ray Observatory in purple and Hubble Space Telescope (HST) data
|
||||
showing optical emission from oxygen ions in orange. The main image is a larger
|
||||
view showing optical and X-ray data from the Kitt Peak National Observatory and
|
||||
ESA's XMM-Newton, respectively. In this image the optical data show emission
|
||||
from oxygen (orange) and hydrogen (green and blue), and X-ray emission is
|
||||
colored purple.
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@image
|
||||
|
|
@ -479,11 +522,8 @@ license_id: CC-PDDC
|
|||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-527.jpg
|
||||
astropix_ids: chandra|527
|
||||
|
||||
credits> X-ray: NASA/CXC/NRC/C.Cheung et ; This composite image shows GB
|
||||
1428+4217, a quasar that contains the most distant X-ray jet ever observed. This
|
||||
view contains X-...
|
||||
credits> X-ray: NASA/CXC/NRC/C.Cheung et al; Optical: NASA/STScI; Radio: NSF/NRAO/VLA
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@scene
|
||||
|
|
@ -492,9 +532,13 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-527L{1}X{2}Y{3}.pn
|
|||
outgoing_url: https://chandra.harvard.edu/photo/2012/gb1428/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-527.jpg
|
||||
|
||||
text> GB 1428+4217
|
||||
text> This composite image shows the most distant X-ray jet ever observed. X-ray
|
||||
data from NASA's Chandra X-ray Observatory are shown in blue, radio data from
|
||||
the NSF's Very Large Array are shown in purple and optical data from NASA's
|
||||
Hubble Space Telescope are shown in yellow. The jet was produced by a quasar
|
||||
named GB 1428+4217, or GB 1428 for short, and is located 12.4 billion light
|
||||
years from Earth.
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@image
|
||||
|
|
@ -504,11 +548,8 @@ license_id: CC-PDDC
|
|||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-528.jpg
|
||||
astropix_ids: chandra|528
|
||||
|
||||
credits> X-ray (NASA/CXC/SAO/A.Prestwich ; NGC 922 was formed by the collision
|
||||
between two galaxies one seen in this composite image (where X-rays from Chandra
|
||||
are red and...
|
||||
credits> X-ray (NASA/CXC/SAO/A.Prestwich et al); Optical (NASA/STScI)
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@scene
|
||||
|
|
@ -517,9 +558,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-528L{1}X{2}Y{3}.pn
|
|||
outgoing_url: https://chandra.harvard.edu/photo/2012/ngc922/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-528.jpg
|
||||
|
||||
text> NGC 922
|
||||
text> The ring galaxy NGC 922 is seen in this composite image containing X-rays
|
||||
from NASA's Chandra X-ray Observatory (red) and optical data from the Hubble
|
||||
Space Telescope (appearing as pink, yellow and blue). NGC 922 was formed by the
|
||||
collision between two galaxies — one seen in this image and another located
|
||||
outside the field of view. This collision triggered the formation of new stars
|
||||
in the shape of a ring. Some of these were massive stars that evolved and
|
||||
collapsed to form black holes.
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@image
|
||||
|
|
@ -529,11 +575,8 @@ license_id: CC-PDDC
|
|||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-529.jpg
|
||||
astropix_ids: chandra|529
|
||||
|
||||
credits> NASA/CXC/Ohio State Univ./C.Grie; This multiwavelength image of the
|
||||
galaxy NGC 3627 contains X-rays from Chandra (blue), infrared data from Spitzer
|
||||
(red), and opt...
|
||||
credits> NASA/CXC/Ohio State Univ./C.Grier et al.; Optical: NASA/STScI, ESO/WFI; Infrared: NASA/JPL-Caltech
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@scene
|
||||
|
|
@ -542,9 +585,14 @@ image_url: http://wwtfiles.blob.core.windows.net/vamp/Chandra-529L{1}X{2}Y{3}.pn
|
|||
outgoing_url: https://chandra.harvard.edu/photo/2012/ngc3627/
|
||||
thumbnail: http://wwtfiles.blob.core.windows.net/vamp/thumb-Chandra-529.jpg
|
||||
|
||||
text> NGC 3627
|
||||
text> The spiral galaxy NGC 3627 is located about 30 million light years from
|
||||
Earth. This composite image includes X-ray data from NASA's Chandra X-ray
|
||||
Observatory (blue), infrared data from the Spitzer Space Telescope (red), and
|
||||
optical data from the Hubble Space Telescope and the Very Large Telescope
|
||||
(yellow). The inset shows the central region, which contains a bright X-ray
|
||||
source that is likely powered by material falling onto a supermassive black
|
||||
hole.
|
||||
|
||||
wip: yes
|
||||
---
|
||||
|
||||
@image
|
||||
|
|
|
|||
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