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Progenitors of Type Ib Supernovae

Published online by Cambridge University Press:  03 August 2017

Nino Panagia  and
Victoria G. Laidler
Nino Panagia
Affiliation:
Space Telescope Science Institute
Victoria G. Laidler
Affiliation:
Astronomy Programs, Computer Sciences Corporation.

Abstract

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We argue that the progenitors of type Ib supernovae are moderately massive stars (M ~ 7 M⊙) in binary systems whereas the hypothesis that they originate from very massive stars (M > 20 M⊙) is not consistent with the observational evidence on SNIb.

Type
Session VII. Evolution
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 567 - 570
Copyright
Copyright © Kluwer 1991 

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