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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 (...) »
|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.|
(Reusing this file)
Images credited first to NASA/CXC are in the 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.)
|Orientation of image||1|
|Image resolution in width direction||300|
|Image resolution in height direction||300|
|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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