... coefficient for the larger star (annular eclipse) is determined more certainly: x1 ... Analysis of the main minimum (annular eclipse) indicates that the limb-darkening ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/Err_Estimated_Par_2_eng.pdf -- 881.9 Кб -- 21.07.2009 Похожие документы
... An important advantage of eclipses of stars by exoplanets for determining stellar limb-darkening coefficients is that reflection and ellipsoidal effects are negligible and the eclipse is annular, with a relatively small radius for the eclipsing planet. ...
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Ссылки http://lnfm1.sai.msu.ru/~marat/articles/eng/HD_209458_eng.pdf -- 765.2 Кб -- 17.11.2010 Похожие документы
... In deep HST/WFPC2 images, these objects are confined to an annular distribution closely corresponding to the galaxy's isophotes (Larsen & Brodie 2000). ...
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Ссылки http://lnfm1.sai.msu.ru/~rastor/Books/Brodie&Strader_ARAA-ExtragalGC.pdf -- 1050.9 Кб -- 11.05.2010 Похожие документы