... 80 6 5 M. G. Mingaliev et al.: ... Jy/K 4 3 2 1 0 25 30 35 40 45 50 55 60 25 30 35 40 ... 3.9 GHz), Jy 1.00 1.05 3.35 1.01 0.74 3.69 0.44 S ... errors of Tant measurements, m The specifics of ... 0. 0. 0. M. G. Mingaliev et al.: ...
... 80 M. G. Mingaliev et al.: ... the NCP region n c = 3.9 GHz 25 30 35 40 45 50 55 60 0 1 2 3 4 ... 8 J0410+769 1.14 1.77 2.23 3.35 4.49 J0626+820 0.31 0.56 0.74 1 ... The errors of T ant measurements, #m The specifics of the RATAN ...
... M. E., 2005, MNRAS, 359, 53L Begum, A, Chengalur, J.N., Karachentsev, I. D., Kaisin ... M., 2007, A&A, 464, 859 Schaye, J., 2004, ApJ, 609, 667 simon, J. D. & Geha, M ...
... m/H] < -1) within 250 p c from the Sun and with prop er motions µ 0.2 /yr, made with ... 0.425 0.425 0.424 m 0.4 4.3 1.4 0.94 0.7 1.34 0.9 m / 800/100 800/100 800/100 550/20 ...
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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
... These analyzers split beams by 4.5 mm, that corresponds to 5 seconds of arc at the 6-m telescope spectrograph slit. ... Such splitting allows to get well widened (up to 0.35 mm) spectra at the Il-nd caaera of HSS with a reciprocal linear ...
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Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/1987/1987_p13-p22.pdf -- 93.6 Кб -- 24.02.2010 Похожие документы