When GRB afterglows get softer, hard components come into play
A. MorettiINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy e-mail: [email protected]R. MarguttiINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy e-mail: [email protected]F. PasottiINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy e-mail: [email protected]A. P. BeardmoreUniversity of Leicester, LE1 7RH, UKS. CampanaINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy e-mail: [email protected]G. ChincariniINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy e-mail: [email protected]S. CovinoINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy e-mail: [email protected]O. GodetUniversity of Leicester, LE1 7RH, UKC. GuidorziINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy e-mail: [email protected]J. P. OsborneUniversity of Leicester, LE1 7RH, UKP. RomanoINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy e-mail: [email protected]G. TagliaferriINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy e-mail: [email protected]
2007en
ABI
Abstract
Aims.We aim to investigate the ability of simple spectral models to describe the early afterglow emission of GRBs.
Identifiers
Citations and references
Cited by 20 references