... A supermassive black hole of 2.45 Ѕ 106 M is another candidate as a source of ... a longer capture time 106 years, by taking vs = 102 km/s and Mbh = 2.45 Ѕ 106 M ... M., and Varshalovich, D. 2005, MNRAS, 1377, 1386 [24] Crannell, C.J., Joyce, G ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/A06_Dogiel01-05Apr07_00:55:03.pdf -- 130.8 Кб -- 04.04.2007 Похожие документы
... Subsequent optical observations revealed a 2.6 day binary period [1], and successfully determined the mass of the compact object and mass-donating star as 5.5 - 7.9 M and 1.7 - 3.3 M , respectively [45]. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/F05_Takahashi01-14Jan07_20:06:21_bandw.pdf -- 360.9 Кб -- 18.01.2007 Похожие документы
... to - observation, tS - seed, M BH ( to ) =M BH ( tS ) L 1 - to - t S exp ; = , LEdd Mc 2 = = 0.45 в 109 yrs Salpeter Time (M/ Begelman) LEdd B ( seed ) = BH ( 1 - ( to - t S ) to ) exp 2 M seed Two most popular accretion models: 102 M , M seed 103 M . ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/presentations/25.12.2007/01-gnedin.pdf -- 1147.6 Кб -- 30.01.2008 Похожие документы
... p, M = 1 - 1.3 в 1010 M (pp, p. [45]), L1760 /M = 0.9 - 1.2 в 1027 p//M . p 2:1, p 1760 (3.7 ± 0.2) в 1037 p -1 . ... Monthly Notices of the Royal Astronomical So ciety, 373, 45 [53] Fenimore, E. E., Cannon T. M., 1981 Applied Optics, 20, 1858 ...
... t o - observation, t S - seed, M BH ( to ) 9 =M BH ( tS ) L 1 - to - t S exp ;= LEdd , Mc 2 = = 0.45 в 10 LEdd B ( seed ) = BH yrs Salpeter Time (M/ Begelman) ( 1 - ( to - t S ) to ) exp 2 Two most popular accretion models: M seed 102 M , M seed 103 M . ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Gnedin.pdf -- 930.6 Кб -- 26.01.2011 Похожие документы