... Modernization of the BAO NAS RA 1-m Schmidt Telescope . ... The modernization of the 1-m Schmidt telescope of the Byurakan Astrophysical ... of the Byurakan Astrophysical Observatory 1-m Schmidt Telescope, SMT-2015 Conference ...
... 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
... The atmospheric muon data gives m 2 2 - m1 2 = 0.001 to 0.01 eV 2 . ... M = 0.28 +/- 0.08 for a flat Omega M + lambda = 1 model, and Omega M = -0.3 +/- 0.17 ... 14 nW/m 2 /sr is about 1.4 m bol =10 th magnitude stars per square degree ...
... e integratio n for Eq u o n th e 1.0 m telescop e o f th e Simeiz Statio n o f th e ... e rapi d declin e i n th e RVs durin g 1994-199 5 fro m +1 6 k m s t o -0. 9 k m s ...
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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
... объектов характеризуется низкой светимостью (M B =-13 -18 m ), малыми линейными размерами 1-10 кпк, голубым показателем цвета ( B - V ) от 0.1m до 0.5 m , низкой металличностью O/H=(1/50 1/3) O/H , высоким содержанием HI и часто наличием WR-особенностей ...
... sources in our Kband speckle image (see Table 1). 1" 2.09 µm Figure 1: Pseudocolor representation of our K # band image of K3 ... North is up and east is to the left. Only for the 10 µm source STHO 1 we can see no counterpart in our Kband image. ...
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Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2006/2005_k3-50a_dina4.ps -- 611.5 Кб -- 24.02.2010 Похожие документы
... For Comet C/2010 S1 (LINEAR), the dust can be presented as aggregates with a characteristic radius of about 1m consisting of ~1000 spherical monomers with a radius of 0.1m and a refractive index of 1.65 0.05 (Fig.2). ...
... of the brighter objects were imaged with the 1.0 m and TI CCD and have a field of 87 ... galaxies were not observed with the 1.0 m telescope, and for these we reproduce 100 ...
... Zeeman echell e spectr a obtaine d wit h CEG S spectrograp h of SAO 1m telescope . Th e dat a reductio n D.N . ... a take n wit h th e coud e spectrograp h CEG S o f th e 1m telescop e o f th e Specia l Astrophysica l Observator y for th e ...
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Ссылки http://www.sao.ru/hq/lizm/conferences/pdf/1999/2000_2_p90-p90.pdf -- 5.4 Кб -- 24.02.2010 Похожие документы