... to be discovered with component magnitude differences m5 at the diffraction-limited ... 5 References C. Allen, A. Poveda and M. A. Herrera, A&A 356, 529 (2000). ... 280.5 82.9 174.8 208.0 143 139 137 193.2 192.9 193.3 287.0 286.9 286.9 37.6 37.4 37 ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2008/AstBu_63_278.pdf -- 229.6 Кб -- 24.02.2010 Похожие документы
... masses of the three brightest objects IRS 3 A, B, and C to be in the range 515 M ... m:s] -06:22:56.29 -06:22:55.49 -06:22:55.42 -06:22:54.28 -06:22:55.23 -06:22:56.36 J ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2002/2002A&A_392_945P.pdf -- 443.6 Кб -- 24.02.2010 Похожие документы
... долгота . -02 h 46 m 22.1 s или -41 о 35' 31".5 . выcота над уpовнем моpя . 970 м . ... m 2.000 ... Трушкин) . A_eff( 2.7cm) = 3.072*H + 360.5m 2 ( 4 o - 80 o ) . ...
... 3 corresponds at first (i.e., for small masses 0.5M) to neutron stars, and then to neutron stars with a growing (with further ... Zh 16 (No. 10), 954. Krivoruchenko, M. I.: 1987, Pis'ma v ZhETF 46, 5. ...
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... SAO RAS 6-m telescope observations In references: 5 confirmed polar rings (including SPRC-7 observed at the 6 m telescope 2010: 5 confirmed polar rings, 1 case of overlap 2011: + 4 confirmed polar rings "The best" objects with known gas/stars kinematics ...