Outflow from Protostars and Angular Momentum Transfer
نویسندگان
چکیده
منابع مشابه
Outflow from YSO and Angular Momentum Transfer
Dynamical contraction of a slowly-rotating magnetized cloud is studied using the magnetohydrodynamical (MHD) simulations. In the isothermal stage (n ∼ < nA ∼ 10 cm), the cloud evolves similarly to that expected from Larson-Penston self-similar solution and experiences the run-away collapse. However, after the central density exceeds ∼ nA, an accretion disk is formed around the adiabatic core. J...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 2001
ISSN: 0074-1809
DOI: 10.1017/s007418090022545x