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Stellar mass loss in late B type supergiants

✍ Scribed by S. Gilheany


Book ID
103498119
Publisher
Elsevier Science
Year
1991
Tongue
English
Weight
691 KB
Volume
34
Category
Article
ISSN
0083-6656

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## Abstract Massive stars are of interest as progenitors of supernovae, i.e. neutron stars and black holes, which can be sources of gravitational waves. Recent population synthesis models can predict neutron star and gravitational wave observations but deal with a fixed supernova rate or an assumed