... disk parameters of R Leo by fitting the following artificial (i.e. non-physical ... disk Uniform disk 1.2 673nm observation 1.0 0.8 0.6 0.4 0.2 0.0 0 5 10 15 20 25 30 ...
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... Several theoretical studies (e.g. Papaloizou & Terquem 1995; Terquem 1998; Bate et al. 2000) have considered the dynamics of a protostellar disk in a binary system where the disk is misaligned with the orbital plane of the binary. ...
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Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2002/2002A&A_381_905W.pdf -- 418.9 Кб -- 24.02.2010 Похожие документы
... Bjorkman K.S., Chentsov E.L., Klochkova V.G. Be binaries with warm dust and exotic high-luminosity A-F emissilon line stars ... Klochkova V.G. The chemical composition of the disk and halo stars. Izvestija SAO, 1991, v.34, p.5-30. ...
... is not depleted by selective separation processes onto dust grains (Bond 1992 ... element which is not depleted by dust-gas separation, for IRAS04296 is close to the ... It may be part of the old disk population. ...
... 7 of the object suggest that it belongs to the Galactic disk population. ... However, both in disk F supergiants (Klochkova and Panchuk 1988a) and in HD 331319 ... intense mass transfer between the atmosphere and the circumstellar gasdust envelope ...
... and their companions are obscured from us by dust clouds, which create a strong and ... and filaments are scattered throughout the galaxy disk, but more than half of the ... In its central part small dust clouds are visible. ...