REM observations of GRB 060418 and GRB 060607A: the onset of the afterglow and the initial fireball Lorentz factor determination
| dc.creator | Molinari, E. | |
| dc.creator | Vergani, S. D. | |
| dc.creator | Malesani, D. | |
| dc.creator | Covino, S. | |
| dc.creator | D'Avanzo, P. | |
| dc.creator | Chincarini, G. | |
| dc.creator | Zerbi, F. M. | |
| dc.creator | Antonelli, L. A. | |
| dc.creator | Conconi, P. | |
| dc.creator | Testa, V. | |
| dc.creator | Tosti, G. | |
| dc.creator | Vitali, F. | |
| dc.creator | D'Alessio, F. | |
| dc.creator | Malaspina, G. | |
| dc.creator | Nicastro, L. | |
| dc.creator | Palazzi, E. | |
| dc.creator | Guetta, D. | |
| dc.creator | Campana, S. | |
| dc.creator | Goldoni, P. | |
| dc.creator | Masetti, N. | |
| dc.creator | Meurs, E. J. A. | |
| dc.creator | Monfardini, A. | |
| dc.creator | Norci, L. | |
| dc.creator | Pian, E. | |
| dc.creator | Piranomonte, S. | |
| dc.creator | Rizzuto, D. | |
| dc.creator | Stefanon, M. | |
| dc.creator | Stella, L. | |
| dc.creator | Tagliaferri, G. | |
| dc.creator | Ward, P. A. | |
| dc.creator | Ihle, G. | |
| dc.creator | Gonzalez, L. | |
| dc.creator | Pizarro, A. | |
| dc.creator | Sinclair, P. | |
| dc.creator | Valenzuela, J. | |
| dc.date | 2006-12-20 | |
| dc.date | 2007-04-24 | |
| dc.date.accessioned | 2026-07-07T11:00:32Z | |
| dc.date.available | 2026-07-07T11:00:32Z | |
| dc.description | Gamma-ray burst (GRB) emission is believed to originate in highly relativistic fireballs. Currently, only lower limits were securely set to the initial fireball Lorentz factor Gamma_0. We aim to provide a direct measure of Gamma_0. The early-time afterglow light curve carries information about Gamma_0, which determines the time of the afterglow peak. We have obtained early observations of the near-infrared afterglows of GRB 060418 and GRB 060607A with the REM robotic telescope. For both events, the afterglow peak could be clearly singled out, allowing a firm determination of the fireball Lorentz of Gamma_0 ~ 400, fully confirming the highly relativistic nature of GRB fireballs. The deceleration radius was inferred to be R_dec ~ 10^17 cm. This is much larger than the internal shocks radius (believed to power the prompt emission), thus providing further evidence for a different origin of the prompt and afterglow stages of the GRB. | |
| dc.description | 6 pages, 3 color figures, 3 tables (including two online); discussion significantly extended, results unchanged; accepted for publication in A&A Letters | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0612607 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0612607 | |
| dc.identifier | Astron.Astrophys.469:L13-L16,2007 | |
| dc.identifier | doi:10.1051/0004-6361:20077388 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/187697 | |
| dc.subject | Astrophysics | |
| dc.title | REM observations of GRB 060418 and GRB 060607A: the onset of the afterglow and the initial fireball Lorentz factor determination | |
| dc.type | text |