Magnetospheric accretion and pre-main-sequence stellar masses
نویسندگان
چکیده
منابع مشابه
Accretion in the ρ - Oph pre - main sequence stars ⋆
Aims. The aim of this paper is to provide a measurement of the mass accretion rate in a large, complete sample of objects in the core of the star forming region ρ Oph. Methods. The sample includes most of the objects (104 out of 111) with evidence of a circumstellar disk from mid-infrared photometry; it covers a stellar mass range from about 0.03 to 3 M⊙ and it is complete to a limiting mass of...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1998
ISSN: 0035-8711,1365-2966
DOI: 10.1046/j.1365-8711.1998.01855.x