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
Hauptverfasser: Uhm, Z. Lucas, Zhang, Bing
Format: Artikel
Sprache:eng
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