... to P( k) can constrain h M , 8 · Growth of perturbations governs cluster evolution ... 0.21 ± 0.05; 8 = 0.77 ± 0.03 · Mtot = M b в M / b в ; 0.93; small trend in ( M ...
... of Technology, USA (3)Aryabhatta Research Institute of Observational Sciences (ARES), India , , 21-24 , 2010 SN2009de SN Ib, Ic IIb - «stripped-envelope» supernovae: , / (WR- ) - (progenitors) 8 - 140 M : MV -20.0 (), MV -17.8 () (Richardson et al ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/22/Fatkhullin.pdf -- 1182.2 Кб -- 26.01.2011 Похожие документы
... ISM they obtained a range 0.7 2.8M , based on the Salpeter IMF (0.1 M - 40 M ... as well, if the lower mass limit for supernovae is 8M instead of 10 M (e.g., [17 ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B07_Hartmann01-07May07_12:04:00.pdf -- 279.4 Кб -- 07.05.2007 Похожие документы
... 2 shows density profiles for three neutron star models with M = 1.8, 1.4, and 0.5 M ... neutron stars (left) and bare strange stars (right) of masses M =0.5, 1.4, and 1.8M ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/H01_Yakovlev01-06Jun07_18:36:08.pdf -- 218.4 Кб -- 06.06.2007 Похожие документы