Accretion disks in luminous young stellar objects
作者： M. T. Beltrán , W. J. de Wit
DOI: 10.1007/S00159-015-0089-Z
关键词:
摘要: An observational review is provided of the properties accretion disks around young stars. It concerns primordial intermediate- and high-mass stellar objects in embedded optically revealed phases. The were derived from spatially resolved observations and, therefore, predominantly obtained with interferometric means, either radio/(sub)millimeter or optical/infrared wavelength regions. We make summaries comparisons physical properties, kinematics, dynamics these circumstellar structures delineate trends where possible. Amongst others, we report on a quadratic trend mass rates T Tauri stars to highest systematic difference infall rates.
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