| dc.contributor.author | Schulze, S. | |
| dc.contributor.author | Zhang, B. | |
| dc.contributor.author | Kann, D. A. | |
| dc.contributor.author | Oates, S. | |
| dc.contributor.author | DE PASQUALE, Massımılıano | |
| dc.date.accessioned | 2022-02-18T10:28:43Z | |
| dc.date.available | 2022-02-18T10:28:43Z | |
| dc.identifier.citation | DE PASQUALE M., Schulze S., Kann D. A. , Oates S., Zhang B., "PHYSICAL PROPERTIES OF RAPIDLY DECAYING AFTERGLOWS", Fall Gamma Ray Burst Symposium on 15 years of Gamma-Ray Bursts afterglows: Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe, Malaga, İspanya, 8 - 12 Ekim 2012, cilt.61, ss.217-221 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_9fc6c975-853b-48eb-aa79-8bc53a3bda37 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/179321 | |
| dc.identifier.uri | https://doi.org/10.1051/eas/1361032 | |
| dc.description.abstract | We analyze a sample of Swift X-ray and optical GRB afterglows which were chosen so as to reduce selection effects against the weakest events. We tentatively identify important differences in GRBs that show a fast decay with respect to the average GRB, in particular a tendency for the more energetic bursts to have a steeper afterglow decline. An explanation to this finding could be bursts in a wind environment are on average more energetic than bursts occurring in a constant density medium. | |
| dc.language.iso | eng | |
| dc.subject | Physics and Astronomy (miscellaneous) | |
| dc.subject | General Physics and Astronomy | |
| dc.subject | Space and Planetary Science | |
| dc.subject | Astronomy and Astrophysics | |
| dc.subject | Physical Sciences | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler | |
| dc.subject | Fizik | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Uzay bilimi | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.title | PHYSICAL PROPERTIES OF RAPIDLY DECAYING AFTERGLOWS | |
| dc.type | Bildiri | |
| dc.contributor.department | University Of Nevada, Las Vegas , Fen Fakültesi , Astronomi Ve Uzay Bilimleri Bölümü | |
| dc.identifier.volume | 61 | |
| dc.contributor.firstauthorID | 3380734 | |