Speaker
Mr
Takashi Moriya
(IPMU, University of Tokyo)
Description
We investigate the effect of non-steady dense mass loss on the shock breakout in
dense wind. We found that the effect of the dense wind from non-steady mass loss can
account for two types of interaction-powered luminous supernovae: 06gy-like LSNe
which show the narrow emission lines from wind and 08es-like LSNe which do not
show them.
Primary author
Mr
Takashi Moriya
(IPMU, University of Tokyo)