Rising optical afterglows seen by TAROT
| dc.creator | Gendre, B. | |
| dc.creator | Klotz, A. | |
| dc.creator | Stratta, G. | |
| dc.creator | Preger, B. | |
| dc.creator | Piro, L. | |
| dc.creator | Pelangeon, A. | |
| dc.creator | Galli, A. | |
| dc.creator | Cutini, S. | |
| dc.creator | Corsi, A. | |
| dc.creator | Boer, M. | |
| dc.creator | Atteia, J. L. | |
| dc.date | 2008-10-02 | |
| dc.date.accessioned | 2026-07-07T10:07:05Z | |
| dc.date.available | 2026-07-07T10:07:05Z | |
| dc.description | We present the multi-wavelength study of those gamma-ray bursts observed by TAROT. These events are characterized by the presence at early time of a rising in their optical light curves lasting a few hundred of seconds. In one case (GRB 060904B), a flare occurs at similar time in the X-ray band, while in the other cases the X-ray light curves appear smooth during the optical rise. We investigate the possible nature of this behavior and conclude th at a multi-component emission is mandatory to explain the optical-to-X-ray afterglow. | |
| dc.description | 2 pages, proceeding of a poster presented at the journees de la SF2A | |
| dc.identifier | https://arxiv.org/abs/0810.0406 | |
| dc.identifier | http://arxiv.org/abs/0810.0406 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/170511 | |
| dc.subject | Astrophysics | |
| dc.title | Rising optical afterglows seen by TAROT | |
| dc.type | text |