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Luminosities of FBS late type M stars

✍ Scribed by H. V. Abrahamyan


Book ID
106354671
Publisher
Springer
Year
2007
Tongue
English
Weight
80 KB
Volume
50
Category
Article
ISSN
0571-7256

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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