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Progenitors of Low-redshift Gamma-Ray Bursts

The bimodal distribution of the observed duration of gamma-ray bursts (GRBs) has led to the identification of two distinct progenitors; compact star mergers, comprising either two neutron stars (NSs) or an NS and a black hole, for short GRBs (SGRBs), and the so-called collapsars for long GRBs (LGRBs...

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Detalles Bibliográficos
Principais autores: Vahé Petrosian, Maria G. Dainotti
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Letters
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Acceso en liña:https://doi.org/10.3847/2041-8213/ad2763
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