Speaker
Dr
Melina Bersten
(IPMU)
Description
We present a model for the Type Ib SN 2008D, associated with the X-ray
Flash 080109, which assumes a double-peaked 56Ni
distribution. This assumption is fundamental to
explain the plateau observed in the light curve a few days after the
explosion. The presence of this high-velocity
radioactive material may be caused by the formation of jets during the
explosion. We briefly discuss the alternative scenarios that have been
suggested for this supernova.
Primary author
Dr
Melina Bersten
(IPMU)
