Difference between revisions of "File:Ngc281 compare.jpg"

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Image title	This composite image of NGC 281 contains X-ray data from Chandra (purple) with infrared observations from Spitzer (red, green, blue). The high-mass stars in NGC 281 drive many aspects of their galactic environment through powerful winds flowing from their surfaces and intense radiation that heats surrounding gas, "boiling it away" into interstellar space. This process results in the formation of large columns of gas and dust, as seen on the left side of the image. These structures likely contain newly forming stars. The eventual deaths of massive stars as supernovas will also seed the galaxy with material and energy.
Author	Chandra X-ray Observatory Center
Date and time of data generation	28 September 2011
Width	1,369 px
Height	1,024 px
Bits per component	1 0 256
Compression scheme	LZW
Pixel composition	RGB
Orientation	Normal
Number of components	3
Horizontal resolution	37.5 dpi
Vertical resolution	0.72818888888889 dpi
Data arrangement	chunky format
File change date and time	5 Macintosh
Exif version	2.21
Color space	sRGB
Unique ID of original document	uuid:778C1DD3D587DC11926FA4AE925315AB
Date and time of digitizing	07:35, 9 May 2011
Software used	Adobe Photoshop CS5 Macintosh
Date metadata was last modified	12:05, 22 August 2012
Source	Chandra X-ray Observatory
Credit/Provider	X-ray: NASA/CXC/CfA/S.Wolk; IR: NASA/JPL/CfA/S.Wolk
Headline	A nebula with active star formation about 6,500 light years from Earth.
Short title	Living the High Life
Keywords	NGC 281
Contact information	cxcpub@cfa.harvard.edu http://chandra.harvard.edu 60 Garden St. Cambridge, MA, 02138 USA 617.496.7941
Usage terms	http://chandra.harvard.edu/photo/image_use.html
IIM version	4

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Revision as of 10:02, 16 March 2013 (view source) Powers (talk \| contribs)	Latest revision as of 10:06, 16 March 2013 (view source) Powers (talk \| contribs) (uploaded a new version of "File:Ngc281 compare.jpg")
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