Author： Claeys J. S. W. de Mink S. E. Pols O. R. Eldridge J. J. Baes M.
Publisher： Edp Sciences
E-ISSN： 1432-0746|528|issue|A131-A131
ISSN： 0004-6361
Source： Astronomy & Astrophysics, Vol.528, Iss.issue, 2011-03, pp. : A131-A131
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Abstract
Massive stars that lose their hydrogen-rich envelope down to a few tenths of a solar mass explode as extended type IIb supernovae, an intriguing subtype that links the hydrogen-rich type II supernovae with the hydrogen-poor type Ib and Ic. The progenitors may be very massive single stars that lose their envelope due to their stellar wind, but mass stripping due to interaction with a companion star in a binary system is currently considered to be the dominant formation channel.
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