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Circumstellar interaction of the type Ia supernova 2002ic
DOI: 10.1111/j.1365-2966.2004.08347.x Bibcode: 2004MNRAS.355..627C

Lundqvist, P.; Chevalier, R. A.; Chugai, N. N.

We propose a model to account for the bolometric light curve, the quasi-continuum and the CaII emission features of the peculiar type Ia supernova (SN) 2002ic, which exploded in a dense circumstellar envelope. The model suggests that the SN Ia had the maximum possible kinetic energy and that the ejecta expand in an approximately spherically symmet…

2004 Monthly Notices of the Royal Astronomical Society
INTEGRAL 41
Identifying young gamma-ray burst fossils
DOI: 10.1111/j.1365-2966.2004.07770.x Bibcode: 2004MNRAS.349L..38R

Ramirez-Ruiz, Enrico

The recent reports of temporal and spectral peculiarities in the early stages of some afterglows suggest that we may be wrong in postulating a central engine that becomes dormant after the burst itself. A continually decreasing post-burst relativistic outflow, such as put out by a decaying magnetar, may continue to be emitted for periods of days o…

2004 Monthly Notices of the Royal Astronomical Society
INTEGRAL 20