Winds from Hot Star Disks

Details Winds from Hot Star Disks Winds from Hot Star Disks

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..337..169k&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

Physics

Scientific paper

Disk winds can account for some of the outflow features observed in spectra of a variety of different types of objects. In addition, winds can have a substantial effect on the mass budget of the disk, and can play a role in the evolution of accreting objects. In this article I will review some of the mechanisms which can cause disk winds and describe recent numerical simulations of these winds.

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