SIMBAD references

2000ApJ...537L.127S - Astrophys. J., 537, L127-L130 (2000/July-2)

SN 1998bw at late phases.

SOLLERMAN J., KOZMA C., FRANSSON C., LEIBUNDGUT B., LUNDQVIST P., RYDE F. and WOUDT P.

Abstract (from CDS):

We present observations of the peculiar supernova SN 1998bw, which was probably associated with GRB 980425. The photometric and spectroscopic evolution is monitored up to 500 days past explosion. We also present modeling based on spherically symmetric, massive progenitor models and very energetic explosions. The models allow line identification and clearly show the importance of mixing. From the late light curves, we estimate that ∼0.3-0.9 M☉ of ejected 56Ni is required to power the supernova.

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Journal keyword(s): Gamma Rays: Bursts - Nuclear Reactions, Nucleosynthesis, Abundances - Stars: Supernovae: Individual: Alphanumeric: SN 1998bw

Simbad objects: 2

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