Masses and luminosities of O- and B-type
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M.M. Hohle; R. NeuhΓ€user; B.F. Schutz
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Article
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2010
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John Wiley and Sons
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English
β 408 KB
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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