... YSOs with the PTI and resolved three of them, two TTauri stars and an HAeBe star ... NIR sizes of various HAeBe and TTauri stars appearing in the literature correlates ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2004/2004A&A_413_217S.pdf -- 186.2 Кб -- 01.02.2005 Похожие документы
... jet widths of 30 AU found for microjets from TTauri stars by Dougados et al ... X-ray luminosities and plasma temperatures for TTauri stars are LX /Lbol 10-4 10-3 ... X-ray luminosities, and compare them to those of TTauri stars in IC 348, class I ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2002/2002A&A_392_945P.pdf -- 443.6 Кб -- 03.08.2004 Похожие документы
... between HAeBes and the lowermass TTauri stars, questions such as the existence of ... The TTauri population in the nearby TaurusAuriga Tassociation displays a factor ... A TTauri type companion lies approximately 4 ## to the northeast (LRH97). ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2005/2005AA_431_307.ps -- 712.0 Кб -- 05.05.2009 Похожие документы
... nebula Mz3 ("Ant nebula"), B protoplanetary nebula RAFGL 2688, C WolfRayet star WR124, D LBV star Car, E Herbig Ae/Be stars, F TTauri Using C M F G E N code we constructed the model of the WR156 atmosphere, the parameters are listed in Table ...
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Ссылки http://mavr.sao.ru/hq/ssl/maryeva/WR156_poster_2014_eng.pdf -- 1081.4 Кб -- 16.06.2014 Похожие документы
... 2 3 days at the birth line of TTauri stars because their sizes are a few times ... a very high level of activity of TTauri stars resulting in an intense stellar wind ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p086.pdf -- 775.2 Кб -- 11.08.2011 Похожие документы
... A number of Herbig Ae stars and classical TTauri stars are surrounded by active accretion disks and, probably, most of the ... 2008). The jet frequency appears to be comparable to that for TTauri stars. ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p163.pdf -- 313.0 Кб -- 11.08.2011 Похожие документы
... Introduction DF Tau is one of the most active classical TTauri stars (CTTS) (Herbig & Bell 1988). ... can see that the amplitude of the photometric activity increases as the wavelengths decrease, which is typical of TTauri stars ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2006/shakhovskoj_etal_aua_dftau_2006.pdf -- 535.7 Кб -- 05.05.2009 Похожие документы