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Accretion disks in luminous young stellar objects

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arxiv 1509.08335 v1 pith:F6T6YM2W submitted 2015-09-28 astro-ph.GA astro-ph.SR

Accretion disks in luminous young stellar objects

M.T. Beltran (1) , W.J. de Wit (2) ((1) INAF-Osservatorio Astrofisico di Arcetri , Firenze , Italy , (2) European Southern Observatory , Santiago de Chile , Chile) This is my paper
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keywords accretionmassyoungdisksobjectspropertiesstellarrates
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An observational review is provided of the properties of accretion disks around young stars. It concerns the primordial disks of intermediate- and high-mass young stellar objects in embedded and optically revealed phases. The properties were derived from spatially resolved observations and therefore predominantly obtained with interferometric means, either in the radio/(sub)millimeter or in the optical/infrared wavelength regions. We make summaries and comparisons of the physical properties, kinematics, and dynamics of these circumstellar structures and delineate trends where possible. Amongst others, we report on a quadratic trend of mass accretion rates with mass from T Tauri stars to the highest mass young stellar objects and on the systematic difference in mass infall and accretion rates.

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