Magnetically and Rotationally Challenged Disks: One Model Fits All?

Details Magnetically and Rotationally Challenged Disks: One Model Fits All? Magnetically and Rotationally Challenged Disks: One Model Fits All?

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..337..129b&link_type=abstract

The Nature and Evolution of Disks Around Hot Stars, ASP Conference Series, Vol. 337, Proceedings of a meeting held 7-9 July 2004

Computer Science

1

Scientific paper

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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