... Triggered Star Formation" . It is now well established that massivestars in star forming regions can trigger next generation of star formation. ...
... The neutron-starmasses presented in Fig. 1 are already given in [8], and we do not ... m LR/m. (8) The change of the star's mass m during a single stage in the model with ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/mx_BH_evolution_eng.pdf -- 210.4 Кб -- 23.06.2005 Похожие документы
... For example, for binary systems with optical-starmasses mv = 20-30 M (close to ... For sysI 1.0 tems with optical-starmasses mv = 1-10 M (close to filling their Roche ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/Vr_forma_eng.pdf -- 661.5 Кб -- 22.11.2005 Похожие документы
... A. M. "Evolution of the Masses of Neutron Stars in Binary Systems" Astronomy Reports ... A.M. "On the existence of massive neutron stars" Astrophysics, 2005, Vol.48, Issue 2 ...
... the size of the initially more massivestar exceeds the current distance between the ... The star's mass-loss rate M is very important for two reasons: it substantially ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/mx_M33_X7_eng.pdf -- 648.2 Кб -- 03.03.2009 Похожие документы
... Triggered Star Formation" . It is now well established that massivestars in star forming regions can trigger next generation of star formation. ...
... star formed during the core collapse of a massivestar can lie in the range 1.0-1.8 ... Third, evolutionary computations of neutron-starmasses in binary systems using the ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/mx_2S0921_630_eng.pdf -- 228.5 Кб -- 30.05.2006 Похожие документы
... case, the rate at which the neutron star accumulates mass will be M Mcr it where Mx ... GMx (4) For massivestars, with lifetimes of less than 107 yr, accretion via the ... the magnetic-field strength and the neutron-starmass, shown in Figs. 2 and 3 ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/mx_evolution_eng.pdf -- 266.6 Кб -- 21.02.2005 Похожие документы
... stars are a natural product of the evolution of stars with masses in excess of 10 M ... areas are lower than the star's center-of-mass velocity, and so the mean velocityof ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/NS_OBgiants_eng.pdf -- 331.6 Кб -- 11.02.2004 Похожие документы
... system agrees within the errors with the mean mass of neutron stars, 1.35+0.04 M [28 ... A. Herrero, IAU Symposium 212: A MassiveStar Odyssei: from Main Sequence to ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/mx_4U1700_eng.pdf -- 320.5 Кб -- 23.06.2004 Похожие документы