GRB 011121: A collimated outflow into wind-blown surroundings
| dc.creator | Greiner, J. | |
| dc.creator | Klose, S. | |
| dc.creator | Salvato, M. | |
| dc.creator | Zeh, A. | |
| dc.creator | Schwarz, R. | |
| dc.creator | Hartmann, D. H. | |
| dc.creator | Masetti, N. | |
| dc.creator | Stecklum, B. | |
| dc.creator | Lamer, G. | |
| dc.creator | Lodieu, N. | |
| dc.creator | Scholz, R. D. | |
| dc.creator | Sterken, C. | |
| dc.creator | Gorosabel, J. | |
| dc.creator | Burud, I. | |
| dc.creator | Rhoads, J. | |
| dc.creator | Mitrofanov, I. | |
| dc.creator | Litvak, M. | |
| dc.creator | Sanin, A. | |
| dc.creator | Grinkov, V. | |
| dc.creator | Andersen, M. I. | |
| dc.creator | Cerón, J. M. Castro | |
| dc.creator | Castro-Tirado, A. J. | |
| dc.creator | Fruchter, A. | |
| dc.creator | Fynbo, J. U. | |
| dc.creator | Hjorth, J. | |
| dc.creator | Kaper, L. | |
| dc.creator | Kouveliotou, C. | |
| dc.creator | Palazzi, E. | |
| dc.creator | Pian, E. | |
| dc.creator | Rol, E. | |
| dc.creator | Tanvir, N. R. | |
| dc.creator | Vreeswijk, P. M. | |
| dc.creator | Wijers, R. A. M. J. | |
| dc.creator | Heuvel, E. van den | |
| dc.date | 2003-09-26 | |
| dc.date.accessioned | 2026-07-07T12:00:57Z | |
| dc.date.available | 2026-07-07T12:00:57Z | |
| dc.description | We discover a break in the GRB 011121 afterglow light curve after 1.3 days, which implies an initial jet opening angle of about 9 deg. The SED during the first four days is achromatic, and supports the jet origin of this break. The SED during the supernova bump can be best represented by a black body with a temperature of 6000 K. The deduced parameters for the decay slope as well as the spectral index favor a wind scenario, i.e. an outflow into a circum-burst environment shaped by the stellar wind of a massive GRB progenitor. Due to its low redshift of z=0.36, GRB 011121 has been the best example for the GRB-supernova connection until GRB 030329, and provides compelling evidence for a circum-burster wind region expected to exist if the progenitor was a massive star. | |
| dc.description | 22 pages ApJ style, accepted for publication | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0309733 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0309733 | |
| dc.identifier | Astrophys.J.599:1223-1237,2003 | |
| dc.identifier | doi:10.1086/379606 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/206952 | |
| dc.subject | Astrophysics | |
| dc.title | GRB 011121: A collimated outflow into wind-blown surroundings | |
| dc.type | text |