The low-luminosity tail of the GRB distribution: The case of GRB 980425

F. Daigne; R. Mochkovitch

doi:10.1393/ncc/i2005-10041-5

The low-luminosity tail of the GRB distribution: The case of GRB 980425

F. Daigne
, R. Mochkovitch

École Polytechnique

Institut d’Astrophysique de Paris

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

The association of GRB 980425 with the nearby supernova SN 1998bw at z = 0.0085 implies the existence of a population of GRBs with an isotropic-equivalent luminosity which is about 104 times smaller than in classical cosmic GRBs. We investigate two scenarios to explain the peculiar properties of GRB 980425: a normal (intrinsically bright) GRB seen off-axis or an intrinsically weak GRB seen on-axis.

langue originale	Anglais
Pages (de - à)	283-286
Nombre de pages	4
journal	Nuovo Cimento della Societa Italiana di Fisica C
Volume	28
Numéro de publication	3
Les DOIs	https://doi.org/10.1393/ncc/i2005-10041-5
état	Publié - 1 janv. 2005

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10.1393/ncc/i2005-10041-5

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title = "The low-luminosity tail of the GRB distribution: The case of GRB 980425",

abstract = "The association of GRB 980425 with the nearby supernova SN 1998bw at z = 0.0085 implies the existence of a population of GRBs with an isotropic-equivalent luminosity which is about 104 times smaller than in classical cosmic GRBs. We investigate two scenarios to explain the peculiar properties of GRB 980425: a normal (intrinsically bright) GRB seen off-axis or an intrinsically weak GRB seen on-axis.",

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AB - The association of GRB 980425 with the nearby supernova SN 1998bw at z = 0.0085 implies the existence of a population of GRBs with an isotropic-equivalent luminosity which is about 104 times smaller than in classical cosmic GRBs. We investigate two scenarios to explain the peculiar properties of GRB 980425: a normal (intrinsically bright) GRB seen off-axis or an intrinsically weak GRB seen on-axis.

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The low-luminosity tail of the GRB distribution: The case of GRB 980425

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