TOWARD AN UNDERSTANDING OF GRB PROMPT EMISSION MECHANISM. I. THE ORIGIN OF SPECTRAL LAGS
ABSTRACT Despite decades of investigations, the physical mechanism that powers the bright prompt γ-ray emission from gamma-ray bursts (GRBs) is still not identified. One important observational clue that still has not been properly interpreted is the existence of time lags of broad light curve pulse...
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Veröffentlicht in: | The Astrophysical journal 2016-07, Vol.825 (2), p.97-97 |
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Format: | Artikel |
Sprache: | eng |
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