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• W3048821857 abstract "Abstract The power per logarithmic bandwidth in gamma-ray burst spectra generally increases rapidly with energy through the x-ray range and does not cut off sharply above a few MeV. This spectral form indicates that a very small fraction of the energy from a gamma-ray burst source is emitted at low energies or is reprocessed into x-rays and that the high-energy gamma rays are not destroyed by photon-photon interactions. The implications are that the emission mechanism for the gamma-ray bursts is not synchrotron radiation from electrons that lose most of their energy before being re-accelerated and that either the regions from which the gamma rays are emitted are large compared to the size of a neutron star or the emission is collimated and beamed away from the stellar surface." @default.
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• W3048821857 date "1986-01-01" @default.
• W3048821857 modified "2023-10-17" @default.
• W3048821857 title "Physical Constraints on Models of Gamma-Ray Bursters" @default.
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• W3048821857 doi "https://doi.org/10.1017/s0252921100086140" @default.
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