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File:N 63A- Chandra and Hubble - Heic0507f.tif

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Original file(2,400 × 2,400 pixels, file size: 16.5 MB, MIME type: image/tiff)

Description

Chandra has imaged the glowing shell created by the destruction of a massive star. X-rays from Chandra (blue), combined with optical (green) and radio (red) data, reveal new details in the supernova remnant, LMC N 63A. The X-ray glow is from material heated to about ten million degrees Celsius by a shock wave generated by the supernova explosion. The age of the remnant is estimated to be in the range of 2,000 to 5,000 years.

Credit: X-ray: NASA/CXC/Rutgers/J.Warren et al.; Optical: NASA/STScI/U. Ill/Y.Chu; Radio: ATCA/U. Ill/J.Dickel et al.

Colours & filters
Band       Wavelength     Telescope
X-ray 	                   Chandra
Optical 	           Hubble Space Telescope
Radio 	                   Other
.
Date
Source http://www.spacetelescope.org/images/heic0507f/
Author ESA/Hubble & NASA
Permission
(Reusing this file)
w:en:Creative Commons
attribution
attribution
ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.
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w:en:Creative Commons
attribution
This file is licensed under the Creative Commons Attribution 4.0 International license.
Attribution: ESA/Hubble & NASA
You are free:
  • to share – to copy, distribute and transmit the work
  • to remix – to adapt the work
Under the following conditions:
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7 June 2005

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Date/TimeThumbnailDimensionsUserComment
current11:19, 4 May 2012Thumbnail for version as of 11:19, 4 May 20122,400 × 2,400 (16.5 MB)Fabian RRRR{{Information |Description=Chandra has imaged the glowing shell created by the destruction of a massive star. X-rays from Chandra (blue), combined with optical (green) and radio (red) data, reveal new details in the supernova remnant, LMC N 63A. The X-...
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Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.