The mass of the star formed in a cloud core |
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| Authors: | Takenori Nakano Tetsuo Hasegawa Colin Norman |
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| Institution: | (1) Nobeyama Radio Observatory, National Astronomical Observatory, Japan;(2) Institute of Astronomy, University of Tokyo, Japan;(3) Department of Physics and Astronomy, Johns Hopkins University, USA |
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| Abstract: | The forming star grows by mass inflow from the parent cloud core, mainly through the accretion disk. However, the core matter which has not yet contracted much is seriously disturbed by the activities of the forming star. We consider mass outflow and emission of ultraviolet radiation as such activities and determine the stellar mass as a function of the physical quantities of the parent cloud core. |
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