Gamma-ray bursts 15 years of GRB afterglows : progenitors, environments and host galaxies from the nearby to the early universe

Gamma-ray bursts (GRB) are amongst the most energetic phenomena in the Universe. In 1997 (more than 15 years ago), BeppoSAX allowed the detection of the first GRB X-ray afterglow, leading to the detection of afterglows at other wavelengths (optical, radio) in the following years, probing the cosmolo...

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Detalles Bibliográficos
Otros Autores: Castro-Tirado, A. J. (Alberto J.), editor (editor), Gorosabel, J., editor, Park, I. H., editor
Formato: Libro electrónico
Idioma:Inglés
Publicado: Les Ulis : EDP SCIENCES 2012
[2021]
Colección:EAS Publication Series
Materias:
Ver en Biblioteca Universitat Ramon Llull:https://discovery.url.edu/permalink/34CSUC_URL/1im36ta/alma991009428400006719
Descripción
Sumario:Gamma-ray bursts (GRB) are amongst the most energetic phenomena in the Universe. In 1997 (more than 15 years ago), BeppoSAX allowed the detection of the first GRB X-ray afterglow, leading to the detection of afterglows at other wavelengths (optical, radio) in the following years, probing the cosmological distance scale. There are still many other open issues which still need to be addressed, regarding both theoretical and observational aspects: prompt emission and afterglow physics, progenitors (including Pop III stars), host galaxies, multi-messenger information, etc.
Descripción Física:1 online resource (675 p.)