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Luminosities of the B stars from spectroscopic measurements

✍ Scribed by R.M. Petrie

Publisher
Elsevier Science
Year
1956
Tongue
English
Weight
751 KB
Volume
2
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