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SN 2006gy and the core of its home galaxy, NGC 1260, viewed in x-ray light from the Chandra X-ray Observatory. The NGC 1260 galactic core is on the lo
SN 2006gy and the core of its home galaxy, NGC 1260, viewed in x-ray light from the Chandra X-ray Observatory. The NGC 1260 galactic core is on the lower left and SN 2006gy is on the upper right.
Light curve of SN 2006gy (uppermost intermittent squares) compared with other types of supernovae
Light curve of SN 2006gy (uppermost intermittent squares) compared with other types of supernovae
This diagram illustrates the pair-instability process that astronomers think triggered the explosion in SN 2006gy. A sufficiently massive star can pro
This diagram illustrates the pair-instability process that astronomers think triggered the explosion in SN 2006gy. A sufficiently massive star can produce gamma rays of such high energy that some of the photons convert into pairs of electrons and positrons causing a runaway reaction which destroys the star.
SN2006gy (top right) in infrared
SN2006gy (top right) in infrared
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Illustration of Chandra
Illustration of Chandra
Space Shuttle Columbia, STS-93 launches in 1999
Space Shuttle Columbia, STS-93 launches in 1999
Crew of STS-93 with a scale model
Crew of STS-93 with a scale model
CXO image of the brown dwarf TWA 5B
CXO image of the brown dwarf TWA 5B