SN contributions to GRB lightcurves

Details SN contributions to GRB lightcurves SN contributions to GRB lightcurves

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004nuphs.132..324m&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 132, p. 324-326.

Physics

Nuclear Physics

1

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 whether other SN types might offer alternatives. While several SN types are ruled out, or are unlikely, notably a couple of types `II-bright' could also explain the observations.

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