Modeling X-ray Emission Line Profiles from Massive Star Winds - A Review
Solar and Stellar Astrophysics
2016-07-27 v1
Abstract
The Chandra and XMM-Newton X-ray telescopes have led to numerous advances in the study and understanding of astrophysical X-ray sources. Particularly important has been the much increased spectral resolution of modern X-ray instrumentation. Wind-broadened emission lines have been spectroscopically resolved for many massive stars. This contribution reviews approaches to the modeling of X-ray emission line profile shapes from single stars, including smooth winds, winds with clumping, optically thin versus thick lines, and the effect of a radius-dependent photoabsorption coefficient.
Keywords
Cite
@article{arxiv.1601.00552,
title = {Modeling X-ray Emission Line Profiles from Massive Star Winds - A Review},
author = {Richard Ignace},
journal= {arXiv preprint arXiv:1601.00552},
year = {2016}
}
Comments
to appear in Advances in Space Research