An artist's impression of the stars creating gamma-ray bursts. The
background blue star is the progenitor of a standard long duration
gamma-ray burst. A so-called Wolf-Rayet star, it has a mass ten or more
times the mass of the sun but has a comparable size. The foreground star
is the suggested progenitor of an ultra-long gamma-ray burst (GRB). It
has a mass of perhaps 20 times the sun but is up to a thousand times
larger. In both cases the GRB is produced by a jet punching through the
star, but in the case of the ultra-long GRBs the much larger size of the
star creates a much longer lived jet. Image copyright Mark A. Garlick,
used with permission by the University of Warwick (Credit: Image
copyright Mark A. Garlick, used with permission by the University of
Warwick)
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Strange New Bursts of Gamma Rays Point to a New Way to Destroy a Star
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