Statistics – Computation
Scientific paper
Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.145....1l&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 145, no. 1, June 1988, p. 1-45.
Statistics
Computation
21
Binary Stars, Computational Astrophysics, Elliptical Galaxies, Magnetic Stars, Spiral Galaxies, Stellar Evolution, Gravitational Waves, Monte Carlo Method, Stellar Mass, Stellar Orbits, Stellar Winds, White Dwarf Stars
Scientific paper
The joint evolution of normal and compact stars in binaries of low and moderate masses (≤10 M_sun;) is considered. The classification and analytical description are given for such evolution. The Monte-Carlo simulation of great number of binaries (≡500000) with different initial parameters allows to evaluate the relative amount of binaries of each evolutionary stage in the Galaxy. The simulation of binary evolution in an elliptical galaxy reveals evolutionary properties of a number of type I supernova explosions in ellipticals. The gravitational wave spectrum in the simulated galaxy has also been obtained, the maximum metric strain amplitude h being 10-19.5 at frequences ν ≅ 10-4Hz.
Lipunov Vladimir M.
Postnov Konstantin A.
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