Back to Volume
Paper: Winds from Hot Star Disks
Volume: 337, The Nature and Evolution of Disks Around Hot Stars
Page: 169
Authors: Kallman, T.
Abstract: 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.
Back to Volume