... Model 1: q = M 2 : M 1 = 0.5, e = 0.5, "hot" disk ( с = 0.08), accretion rate = 10 -10 /year. ... Model 2: q = M 2 : M 1 = 0.5, e = 0.5, "warm" disk ( с = 0.05), accretion rate = 3 10 -11 /year. ...
... Diagnostics for AccretionDisks Around UX Ori Stars Based on Balmer, Paschen, and Brackett Lines" , Tambovtseva L. V., Grinin V ... Non-LTE Modeling of AccretionDisks of UX Ori-Type Stars" , Tambovtseva L. V., Grinin V. P.; ASPC 2000, 219, 428 . ...
... the broadening of photospheric lines due to the scattering by the CS dust at the puffed-up inner rim of the accretiondisks ... line arises, for example, in a flattened rotating envelope or accretiondisk, the line profiles of the direct and scattered ...
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Ссылки http://www.gao.spb.ru/personal/sfg/eng/articles/2012/aa19768-12.pdf -- 277.5 Кб -- 02.06.2014 Похожие документы
... Diagnostics for AccretionDisks Around UX Ori Stars Based on Balmer, Paschen, and Brackett Lines" , Tambovtseva, L. V., Grinin ... Non-LTE Modeling of AccretionDisks of UX Ori-Type Stars" , Tambovtseva, L. V., Grinin, V. P.; ASPC 2000, 219, 428 . ...
... disk-wind model consisting of an accretiondisk, which emits the observed continuum ... ob jects such as inner gaseous accretiondisks, dust disks, disk winds, jets, etc ...
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Ссылки http://www.gao.spb.ru/english/personal/sfg/eng/articles/2011/1101.3695v1.pdf -- 1334.8 Кб -- 27.01.2012 Похожие документы