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Sn2006gy light curve
 

 

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Description
English: Original caption: "This graph shows the intrinsic brightness of SN 2006gy and how it changes over time. The graphic also demonstrates how much brighter SN 2006gy is when compared to typical examples of the two main supernova classes. Type Ia supernovas involve the thermonuclear explosion of a white dwarf and type II supernovas are the collapse of a massive star. The famous supernova SN 1987A is also shown. Not only does SN 2006gy get much brighter than other supernovas but it stays very bright for much longer."
Français : « Ce graphique montre la brillance intrinsèque de SN 2006gy et comment celle-ci change dans le temps (...) »
Date Unknown date
Source http://chandra.harvard.edu/photo/2007/sn2006gy/more.html, specifically http://chandra.harvard.edu/photo/2007/sn2006gy/sn2006gy_light_curve.tif
Author NASA/CXC/UC Berkeley/N.Smith et al.
Permission
(Reusing this file)

Images credited first to NASA/CXC are in the public domain.

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Public domain This file is in the public domain because it was created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)

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EXIF data:
File name sn2006gy_light_curve.jpg
Size, bytes 431118
Mime type image/jpeg
Orientation of image 1
Image resolution in width direction 3000000/10000
Image resolution in height direction 3000000/10000
Unit of X and Y resolution 2
Color space information 65535
Exif image width 3000
Exif image length 2025
Software used Adobe Photoshop CS2 Windows
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