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http://star.arm.ac.uk/annrep/annrep2001/node36.html.
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1. EVOLUTION MODELS
Next: MASSES Up: EXTREME HELIUM STARS: PULSATION Previous: STELLAR PROPERTIES . ... Following main-sequence evolution, a red giant star in a close binary system may expand to fill its Roche lobe. ... Although Iben & Tutukov (1984) used this model to account for the EHes, the latter are not binaries (Jeffery et al. ... Final helium-shell flash in a post-AGB star. ... Accretion from the disk onto the surviving WD creates a star with a degenerate CO core and a helium envelope. ... Other models. ...
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Ссылки http://star.arm.ac.uk/~csj/research/ehe_review/node3.html -- 7.9 Кб -- 25.01.2002
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2. Yurij Shokin
Professor Yurij Shokin, born 1943, has been many years with the Computer Center and the Institute of Theoretical and Applied Mechanics (during the directorship of Academician N N Yanenko ) in Novosibirsk's scientific campus Akademgorodok and was director of the computer centre of the Soviet Academy of Sciences, Siberian Division, in Krasnoyarsk. ... He is an affiliate member of IFIP WG 2.5 and a member of the Russian Academy of Sciences. ... Russian Academy of Sciences . Siberian Division . ...
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Ссылки http://star.arm.ac.uk/f77to90/yurij.html -- 3.7 Кб -- 11.09.1996
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