Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-11-03
Astrophys.J.653:L129-L132,2006
Astronomy and Astrophysics
Astrophysics
Accepted for publication on ApJL
Scientific paper
10.1086/510667
We revisit the case of SN2002ic that recently revived the debate about the progenitors of SNeIa after the claim of the unprecedented presence of hydrogen lines over a diluted SNIa spectrum. As an alternative to the previous interpretation, we suggest that SN2002ic actually was a type Ic SN, the core collapse of a massive star which lost its hydrogen and helium envelope. In this scenario the observed interaction with a dense circumstellar material (CSM) is the predictable consequence of the intense mass-loss of the progenitor and/or of the presence of a gas rich environment. With this view we establish a link between energetic SNeIc and highly interacting SNeIIn and add some credits to the proposed association of some SNeIIn to GRBs.
Benetti Stefano
Cappellaro Enrico
Harutyunyan Ararat
Taubenberger Stefan
Turatto Massimo
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