... vt Hu ju "hy~ ji ql z rh ?yp } ji q jhy~ ih jijs jljl h p Vz Fњ ok pyp ljw} h ri vt u ' jlvq ru{s zt T 16 1/2 G 200 M 1/2 20% 1 jm ?l {tr| yzp qHu { | ...
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Ссылки http://jet.sao.ru/hq/ssl/gvard/Panchuk-Odessa2007.20.103-Interf.pdf -- 129.8 Кб -- 01.11.2012 Похожие документы
... It can be easily shown that if the spectrum in the cube FLAT is shifted by 23 channels or its F W H M differs from OBJECT by 20 %, perturbations will then arise with a dispersion of 0.15 0.2 and 0.050.08 of continuum intensity for FP235 and FP501 ...
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Ссылки http://jet.sao.ru/hq/lsfvo/devices/scorpio-2/manuals/0211104.pdf -- 900.1 Кб -- 16.08.2013 Похожие документы
... This might indicate or too close companions (less than 20 mas for the 6m telescope, and 120 mas for the 1m telescope), or too large magnitude di#erence (more than 3 magnitudes), or very bad seeing, or the combination of these factors. ...
... Russian KOI8 . Tuesday, March 5, 14-30 . 1. V.M.Bogod. Modernization of the complex for solar study. Suggestion to develep. 2. ... Suggestions to use spectral radiometers for continuum observations. Wednesday, February 20, 14-30 . 1. Yu.N.Parijskij. ...
... 16 h (galactic latitudes from 45 dg to 90 dg) with the help of RATAN-600 radio telescope with mean angular resolution 2.0'x 20 ... Velocity resolution is 6.3 km/s, r.m.s. noise fluctuation of antenna temperature is 0.1 K . ...
... A. M. 2001, ApJ, 556, 265 Wood, K., Kenyon, S. J., Whitney, B., & Bjorkman, J. E. 1996, ApJ, 458, L79 Zaitseva, G. V., & Lyutyi, V. M. 1976, Variable Stars, 20, 255 Hartigan, P., & Kenyon, S. J. 2003, ApJ, 583, 334 Herbig, G. H., & Bell, K. R. 1988, Lick ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2006/shakhovskoj_etal_aua_dftau_2006.pdf -- 535.7 Кб -- 24.02.2010 Похожие документы