... The translation was initiated by Valentina M.Maxsimova on 2006-01-17 . Valentina M.Maxsimova 2006-01-17. ... The translation was initiated by Valentina M.Maxsimova on 2006-01-17 . Valentina M.Maxsimova 2006-01-17. ...
... Пределом является звездная величина m b =17.0, хотя выборка неполная даже до m b =15.0. ... Pustilnik et al. (1995) исследовали пространственное распределение этой выборки и определили, что она полна до m17m . ...
... and mass, resp., and AK is the 2.2 m dustshell albedo. model V r in T in n0:05 m0:05 AK in (R ) (K) (%) (%) (mas) M 1 0.88 179 1670 99.55 34 0.36 17.8 M 2 0.70 140 1820 98.83 17 0.40 16.3 M 3 0.70 152 1760 0.36 17.5 M 1.1 0.73 159 1740 99.55 34 0.36 ...
... During 2004 and 2005, V532 becomes brighter and reaches 17m in B band (Fig.1). ... Top panel: the spectrum obtained in February 2006 when V532 is 17m .27 in V band. ...
... 95 0.0 0.8 100 mas b 2.12 µm, 10/95, =0.88 100 mas g E 2.12 µm, 10/95, =0.88 0.4 4/96 0.0 B C D A 0.8 0.4 1/97 100 mas c 2.17 µm, 4/96, =0.15 100 mas 2.17 µm, 4/96, =0.15 0.0 0.8 h 0.4 6/98 0.0 0.8 2.19 µm (K), 1/97, =0.61 2.19 µm (K), 1/97, =0.61 100 mas ...
... 3.71 8.78 9.29 9.82 6.74 6.23 6.95 MM 2.90 1.17 2.33 1.71 2.03 1.47 0.84 1.75 2.68 ... the subsequent individual masses of the components are MA = 1.17M and MB = 1.16 M ...
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Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2006/balega_etal_aua_hipparcosbinaries2_2006.pdf -- 386.6 Кб -- 24.02.2010 Похожие документы
... Grunhut et al. also used I U E ultraviolet and ESPaDOnS optical spectroscopy to determine the following physical parameters using the CMFGEN: Teff = 34.5 kK, log(g ) = 4.0 ± 0.2, R = 7.0+2.4 R , -1.8 M = 17+19 M , and log(M ) = -8.85 ± 0.5 M yr-1 . ...
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Ссылки http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p473.pdf -- 332.3 Кб -- 11.08.2011 Похожие документы