... eclipsed satellite. reference frame: astrometric centre of frame: topocenter for ... or eclipsing satellite and n_p is the number of the occulted or eclipsed satellite ...
... eclipsed satellite. reference frame: astrometric centre of frame: topocenter for ... or eclipsing satellite and $n_p$ is the number of the occulted or eclipsed satellite ...
... Solar Activity Monitoring and Forecasting (Ondrejov) and Central European Solar ... Particle Effects in Solar Flares ; 12th European Solar Physics Meeting, Freiburg ... Total Emissivity in Chromospheric Lines in the 17th May 2002 Flare ; 12th European ...
... transit but could be due to an eclipsing binary (EB), either in the background or ... larger than 20 R , observed secondary eclipse, or astrometric motion of the target ...
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Ссылки http://lnfm1.sai.msu.ru/SETI/koi/audio/PNAS-2013-Petigura-1319909110.pdf -- 928.2 Кб -- 18.11.2013 Похожие документы
... A total of 17 spectra at 61006800 A ° with a dispersion of 20 A/mm were obtained. ... A total of 85 spectra were ob° tained: 23 with a dispersion of 39 A/mm obtained ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/mx_CygX1_eng.pdf -- 221.7 Кб -- 17.07.2004 Похожие документы
... sequence position with metallicity is steep near the solar metallicity of [Fe/H] = 0 ... Hence, the mean [Fe/H] of the Cepheid-bearing clusters is solar on average. ...
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Ссылки http://lnfm1.sai.msu.ru/~rastor/Books/Sandage&Tammann_LuminCalibr.pdf -- 1151.8 Кб -- 16.07.2008 Похожие документы