... Spectropolarimetry and modeling of Galactic Wolf-Rayetstar WR156 O LGA M A RY E VA Special Astrophysical Observatory RAS; olga ... According to it, WR156 is the richest hydrogen Wolf-Rayetstar of WN8 type in the Galaxy. ...
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Ссылки http://jet.sao.ru/hq/ssl/maryeva/WR156_poster_2014_eng.pdf -- 1081.4 Кб -- 16.06.2014 Похожие документы
... P.K. ?Spectral Study of the late nitrogen-sequence Wolf-RayetStar FSZ35 in M33 ... Maryeva O.V. ?Modeling Hydrogen-Rich Wolf-RayetStars in M33?, ... O.V. ``Modeling atmospheres of Wolf-Rayetstars'', vol. 17, issue 6, 908-909, Review ...
... radiative transfer modelling of the Wolf-Rayetstar WR 118 B. Yudin1 , Y. Balega2 ... WR 118 is a highly evolved Wolf-Rayetstar of the WC10 subtype surrounded by a ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_379_229Y.pdf -- 168.2 Кб -- 24.02.2010 Похожие документы
... Modeling Hydrogen-Rich Wolf-RayetStars in M33" . Maryeva Olga . ... Spectral study of the late nitrogen-sequence Wolf-Rayetstar FSZ35 in M33" . ... Discovery of a new Wolf-Rayetstar and its ring nebula in Cygnus" . ...
... 233, 133 Polcaro V.F.,Gualandi R., Norci L. 2003, A&A, 411, 193 Romano G. 1978, A&A, 67, 291 Szeifert T. 1996, In: Wolf-RayetStars in the Framework of Stellar Evolution Eds. J.M.Vreux, A.Detal, D.FraipontCaro, E.Gosset and G.Rauw. 33rd Liege Institute ...
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Ссылки http://jet.sao.ru/hq/ssl/maryeva/massive_stars_poster11.pdf -- 303.4 Кб -- 31.10.2013 Похожие документы
... Key words: stars: Wolf-Rayet stars: supergiants stars: massloss stars: individual: IRC +10 420 stars: circumstellar ... star (see Jones et al. 1993 and Oudmaijer et al. 1996), therefore being the only massive object observed until now in its ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_1999/1999A&A_348_805B.pdf -- 387.4 Кб -- 24.02.2010 Похожие документы
... evolution calculations considering convective overshoot have shown how thermal pulses during the post-AGB stage lead to the formation of hydrogen-deficient post-AGB stars with abundance patterns consistent with those observed for Wolf-Rayet central stars ...