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The evolution of the gravitational radiation from stellar components of galaxiesThe evolution is discussed of gravitational waves spectra produced by binary stars, supernova explosions, and coalescences of binary compact stars in outer galaxies. These spectra are integrated over a simple model of the universe to give an estimate of the stochastic gravitational wave background due to astrophysical sources.
Document ID
19920003741
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Lipunov, V. M. (Academy of Sciences (USSR) Moscow, Ussr)
Osminkin, E. YU. (Academy of Sciences (USSR) Moscow, Ussr)
Prokhorov, M. E. (Academy of Sciences (USSR) Moscow, Ussr)
Date Acquired
August 15, 2013
Publication Date
January 1, 1991
Publication Information
Publication: NAS-NRC, High-Energy Astrophysics. American and Soviet Perspectives
Subject Category
Astrophysics
Accession Number
92N12959
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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