Cargando…
What we learn from the afterglow of GRB 021211
The behaviour of the afterglow (AG) of gamma-ray bursts (GRBs) directly provides, in the cannonball (CB) model, information about the environment of their progenitor stars. The well observed early temporal decline of the AG of GRB 021211 is precisely the one predicted in the presence of a progenitor...
| Autores principales: | , , |
|---|---|
| Lenguaje: | eng |
| Publicado: |
2003
|
| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1086/376570 http://cds.cern.ch/record/606204 |