Cargando…
Fireballs and cannonballs confront the afterglow of GRB 991208
Galama et al. have recently reported their follow-up measurements of the radio afterglow (AG) of the Gamma Ray Burst (GRB) 991208, up to 293 days after burst, and their reanalysis of the broad-band AG, in the framework of standard fireball models. They advocate a serious revision of their prior anal...
Autores principales: | Dado, Shlomo, Dar, Arnon, De Rujula, Alvaro |
---|---|
Lenguaje: | eng |
Publicado: |
2002
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0370-2693(03)00593-8 http://cds.cern.ch/record/593774 |
Ejemplares similares
-
The Discovery of a Hyperluminal Source in the Radio Afterglow of GRB 030329
por: Dado, Shlomo, et al.
Publicado: (2004) -
The superluminal motion of Gamma-Ray-Burst sources and the complex afterglow of GRB 030329
por: Dado, Shlomo, et al.
Publicado: (2004) -
What we learn from the afterglow of GRB 021211
por: Dado, S, et al.
Publicado: (2003) -
The Cannonball Model of Gamma Ray Bursts: Lines in the X-Ray Afterglow
por: Dar, Arnon, et al.
Publicado: (2001) -
Optical and X-ray Afterglows in the Cannonball Model of GRBs
por: De Rújula, Alvaro
Publicado: (2002)