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- W4252062033 abstract "Summary A “typical” GRB occurs in a star-forming region of a galaxy at a redshift z~1. In currently popular models, it is caused by the collapse of a massive star which has exhausted its nuclear fuel supply. The star collapses to a black hole threaded by a strong magnetic field, and possibly fed by an accretion torus. Through a variety of processes, electrons are accelerated and gamma-rays, X-rays, optical light, and radio emission ensue, with durations from seconds to years. In this talk, I will review the general observational properties of bursts, their afterglows and host galaxies, and some of the open questions about them." @default.
- W4252062033 created "2022-05-12" @default.
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- W4252062033 date "2005-01-01" @default.
- W4252062033 modified "2023-09-24" @default.
- W4252062033 title "Cosmic Gamma-Ray Bursts: The Big Picture" @default.
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- W4252062033 doi "https://doi.org/10.1017/s0252921100009519" @default.
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