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Paper: Magnetically and Rotationally Challenged Disks: One Model Fits All?
Volume: 337, The Nature and Evolution of Disks Around Hot Stars
Page: 129
Authors: Baade, D.; ud-Doula, A.
Abstract: The disk models presented on the second day of the workshop are summarized. Starting from the joint discussion session following them, some of their strengths and weaknesses are highlighted. The still fairly incomplete empirical classification of disks is also briefly compiled. Special emphasis is given to the challenges resulting from rapid rotation and magnetic fields. Some criteria, that may be used to further enhance models, are developed.
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