2 papers
astro-ph2004
The Effect of Rotational Gravity Darkening on Magnetically Torqued Be Star Disks
J. C. Brown, D. Telfer, Q. Li +3
In the magnetically torqued disk (MTD) model for hot star disks, as proposed and formulated by \citet{cassi02}, stellar wind mass loss was taken to be uniform over the stellar surf…
astro-ph2004
Optically Thick Clumps - Not the Solution to the Wolf-Rayet Wind Momentum Problem?
J C Brown, J P Cassinelli, Q Li +2
The hot star wind momentum problem η= mdot*vinfty/(L/c) >> 1 is revisited, and it is shown that the conventional belief, that it can be solved by a combination of clumping of the w…