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Gamma Ray Burst Afterglow: Supernova Connection
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Gamma Ray Burst Afterglow: Supernova Connection
Credit & Copyright: HST Image: D.W. Fox, J.S. Bloom, S.R. Kulkarni (Caltech), et al.
XMM Result: J.N. Reeves, D. Watson, J.P. Osborne (University of Leicester), et al.
Explanation: What causes the mysterious gamma-ray bursts? Indicated in this Hubble Space Telescope exposure of an otherwise unremarkable field in the constellation Crater, is the dwindling optical afterglow of a gamma-ray burst first detected by the Beppo-SAX satellite on 2001 December 11. The burst's host galaxy, billions of light-years distant, is the faint smudge extending above and to the left of the afterglow position. After rapidly catching the fading x-ray light from the burst with the orbiting XMM-Newton observatory, astronomers are now reporting the telltale signatures of elements magnesium, silicon, sulphur, argon, and calcium - material most likely found in an expanding debris cloud produced by the explosion of a massive star. The exciting result is evidence that the gamma-ray burst itself is linked to a very energetic supernova explosion which may have preceded the powerful flash of gamma-rays by up to a few days.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
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NASA Official: Jay Norris. Specific rights apply.
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& Michigan Tech. U.

Based on Astronomy Picture Of the Day

Publications with keywords: GRB 011211 - gamma-ray burst - supernova
Publications with words: GRB 011211 - gamma-ray burst - supernova
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