... distribution and cannot explain the absence of black holes in the 2 - 5M mass range ... In particular, we show that there is a paucity of black holes with masses 2 - 5M . ...
... arises from accretion power, the estimated primary mass would fall to 3.0-3.5M ... 1.0 M # if the primary is 1.6 M # or 2--2.5M # if the primary is around 3.5--4 M ... Hillenbrand et al. (1992), and one of 4.0 and 2.5M # , following Natta et al ...
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Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2005/2005AA_431_307.ps -- 712.0 Кб -- 24.02.2010 Похожие документы
... mass-loss rate M 1.9 в 10-5M yr-1 , assuming a constant outflow velocity v = 14 km ... envelope, then presently the star would be losing mass at a rate M 6.0 в 10-5M yr-1 ...
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Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2006/menshchikov_etal_aua_lpandromedae_2006.pdf -- 729.5 Кб -- 24.02.2010 Похожие документы
... array, 2562 pixels, sensitivity from 1 to 2.5 µm, frame rate 2 frames/s) through a ... close to the one found by 5 µm interferometric measurements (140150 ; McCarthy 1979 ... 1997; Danchi et al. 1999), and at 11.5 µm (Sudol et al. 1999) 4. ...
... et al. (1994) interferometric 11.5 µm measurements, Burns et al. (1998) observations ... ranging between 1.0 and 1.5M should have a linear photospheric radius ranging from ...
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Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_376_518H.pdf -- 532.0 Кб -- 24.02.2010 Похожие документы
... Eq u ( v sin i < 5 k m s ) an d 4 9 Ca m ( v sin % = 2 2 k m s Th e typica l FOp ... n R V an d th e valu e 1.4 1.5 k m s fro m Wilson' s Genera l Catalo g o f Radia l ...
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Ссылки http://www.sao.ru/hq/lizm/conferences/pdf/1996/1996_p114.pdf -- 48.1 Кб -- 21.04.2010 Похожие документы