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Stellar mass loss in late B-type supergiants

✍ Scribed by S. Gilheany; B. Bates; M. G. Catney; P. L. Dufton

Book ID: 104857202
Publisher: Springer Netherlands
Year: 1990
Tongue: English
Weight: 409 KB
Volume: 169
Category: Article
ISSN: 0004-640X
DOI: 10.1007/bf00640690

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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