Formation Rates of Supernovae Ia and Cataclysmic Binaries as a Function of the Age of Stellar Systems

作者: A. V. Tutukov , L. R. Yungelson

DOI: 10.1007/978-94-011-0335-0_134

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摘要: A model of populations merging binary degenerate dwarfs and cataclysmic binaries (CB) was constructed by means a scenario code. Formation rates both decrease with the age progenitor stellar population. This explains observed trends in SNe Ia novae rates. Higher ratio frequencies elliptical galaxies as compared spiral is explained consequence faster rate relative to formation CB. The shows, that mean dwarf mass zero-age CB changes population from ~ M ⊙ for ages below 108 yr ~O.3M oldest about 1010 yr. Thus, difference between ‘disk’ ‘bulge’ may be result different average their progenitors.

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