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Accretion disks in luminous young stellar objects
The Astronomy and Astrophysics Review ( IF 16.000 ) Pub Date : 2016-01-11 , DOI: 10.1007/s00159-015-0089-z
M. T. Beltrán; W. J. de Wit

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.
更新日期:2016-01-11

 

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