SN contributions to GRB lightcurves

Details SN contributions to GRB lightcurves SN contributions to GRB lightcurves

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ncimc..28..621m&link_type=abstract

Il Nuovo Cimento C, vol. 28, Issue 4, p.621

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Scientific paper

Several of the nearer GRB afterglows (up to z ˜ 1) show bumps in their lightcurves that have been interpreted as contributions from associated SNae. The bumps are customarily modelled like the type-Ic SN 1998bw, but we investigate 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.

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