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      THE EFFECTS OF RADIATIVE TRANSFER ON LOW-MASS STAR FORMATION

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          Mass, luminosity, and line width relations of Galactic molecular clouds

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            Magnetocentrifugally driven flows from young stars and disks. 1: A generalized model

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              Composition and radiative properties of grains in molecular clouds and accretion disks

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                Author and article information

                Journal
                The Astrophysical Journal
                ApJ
                IOP Publishing
                0004-637X
                1538-4357
                September 20 2009
                September 20 2009
                August 26 2009
                : 703
                : 1
                : 131-149
                Article
                10.1088/0004-637X/703/1/131
                dfc6bd69-363f-4b8f-ba2c-14bfe9cb36ad
                © 2009
                History

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