Реферат: To suggest consistent route toward planetesimal and planetary core formation in circumstellar discs we study gravitational instability outcomes in massive multiphase (gas-collisionless bodies) disc. Such unstable massive disc can be formed together with protostar in molecular cloud collapse with increased ratio of solids to gas density. In our calculations we found regimes when low-massive solid bodies subdisc drastically affect global structure formation in the disc, whose mass is constituted mainly by the gas. We demonstrated also that solitary areas of high gas density can concentrate solids, producing multiphase clumps, which can be considered as a cradle of large bodies formation

Библиографическая ссылка: Stoyanovskaya O.P. , Snytnikov V.N.
Numerical Modeling of Gravitational Instability Outcomes in Multiphase Circumstellar Discs
В сборнике Instabilities and Structures in Proto-Planetary Disks. 2013. – ISBN 9782759809837. DOI: 10.1051/epjconf/20134607005 WOS Scopus РИНЦ CAPlusCA OpenAlex

Файлы: Полный текст от издателя

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Опубликована online:

11 апр. 2013 г.

Идентификаторы БД:

Web of science:	WOS:000319936900031
Scopus:	2-s2.0-84876262051
РИНЦ:	20433199
Chemical Abstracts:	2013:655672
Chemical Abstracts (print):	159:137789
OpenAlex:	W2022709720

Цитирование в БД: Пока нет цитирований

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