Hydrodynamical models of clumping beyond 50 stellar radii
Astrophysics
2007-11-14 v1
Abstract
We present one-dimensional, time-dependent models of the clumps generated by the line-deshadowing instability. In order to follow the clumps out to distances of more than 1000 stellar radii, we use an efficient moving-box technique. We show that, within the approximations, the wind can remain clumped well into the formation region of the radio continuum.
Keywords
Cite
@article{arxiv.0711.1939,
title = {Hydrodynamical models of clumping beyond 50 stellar radii},
author = {M. C. Runacres},
journal= {arXiv preprint arXiv:0711.1939},
year = {2007}
}
Comments
International Workshop on clumping in Hot-Star Winds, June 2007, Potsdam, Germany. (3 pages, 2 figures)