Meurs, E. J. A. and Rebelo, M. C. A. (2005) SN contributions to GRB lightcurves. Il nuovo cimento C, 28 (4\5). pp. 621-624. ISSN 1826-9885
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Abstract
Several of the nearer GRB afterglows (up to z ∼ 1) show bumps in their lightcurves that have been interpreted as contributions from associated SNae. Thebumps arecustomarily modelled likethet ype-Ic SN 1998bw, but wein vestigate here, for several low-z GRBs, whether other SN types might offer alternatives. While several SN types are ruled out, or are unlikely, a type “II-bl” could also explain the observations.
| Item Type: | Article |
|---|---|
| Additional Information: | Paper presented at the “4th Workshop on Gamma-Ray Burst in the Afterglow Era”, Rome, October 18-22, 2004. |
| Uncontrolled Keywords: | γ-ray source, γ-ray burst |
| Subjects: | 500 Scienze naturali e Matematica > 520 Astronomia e scienze connesse |
| Depositing User: | Marina Spanti |
| Date Deposited: | 16 Mar 2020 17:42 |
| Last Modified: | 16 Mar 2020 17:42 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/15796 |
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