... Расчеты проводились 21 0 2 4 6 8 h = 90 o cm l = 1 1.5 1.4 1.3 1.2 1.1 1.0 4 3 2 1 x = 1.5m x = 1.0 m x = 0.5m x = 0. m D D D D 4 - 3 - 2 - 1 - H E q 0.5 q 0.5 P 21 (%) Рис. ...
... Parameters of hot comp onents are: M = 34.0 M and 15.5M , Tef f = 39900 K and 31900 K, the distance -- 414±7 p c (Menten et al. 2007), the p erio d of rotation -- 15.426 days (Stahl et al. ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2006/p214.pdf -- 138.8 Кб -- 26.12.2008 Похожие документы
... of 576-m circle of 895 elements (2 x 11.5m), which could use as four independent sectors (225 elements) of that reflector ... latitude (phi) . 43 o 49' 52".75?0".16 . longitude . -02 h 46 m 22.1 s or -41 о 35' 31".5 . hight from sea level . 970 m . ...
... however, ob jects later than M3.5 (Teff 3400 K, M < 0.35M ) are believed to become ... Model parameters: Teff = 3100 K, log g = 5.0, [M/H] = 0.0, v sin i = 2.5 km/s ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p280.pdf -- 567.7 Кб -- 11.08.2011 Похожие документы
... carried out AO observations of NGC 1068 at 3.5 µm (resolution 0.24 ) and 4.8 µm with ... approximately N-S direction coinciding with the 12.5 µm emission found by Bock et al ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2004/2004A&A_425_77.pdf -- 483.6 Кб -- 01.02.2005 Похожие документы
... of elongation of the dust-emitting region at mid-infrared (MIR) wavelengths (5 µm: Hackwell et al. 1982; 11.7 µm and 18.3 µm ... The four bands are recorded simultaneously using two InSb (3.6 µm, 4.5 µm) and two Si:As (5.8 µm, 8.0 µm) detectors. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2006/kraus_etal_aua_ngc7538irs1.5_2006.pdf -- 687.2 Кб -- 05.05.2009 Похожие документы
... System velocity V 0 , km s -1 5.76 0.05 Primary mass, M # 1.28 0.15 Secondary mass ... 54 0.56 0.58 0.6 BV 2.5 3 3.5 4 4.5M V Aa 1.39 Ba 1.32 Ab 1.30 Bb 1.20 2.51 Gyr 2 ...