热星风中变率的 FUSE 观测
天体物理学
2007-05-23 v1
摘要
New constraints on the large-scale wind structures responsible for discrete absorption components are obtained from far-ultraviolet time-series observations of O supergiants in the Large Magellanic Cloud.
引用
@article{arxiv.astro-ph/0410082,
title = {FUSE Observations of Variability in Hot-Star Winds},
author = {A. W. Fullerton and D. L. Massa and R. K. Prinja and I. D. Howarth and A. J. Willis and S. P. Owocki},
journal= {arXiv preprint arXiv:astro-ph/0410082},
year = {2007}
}
备注
3 pages, 1 figure; To appear in proceedings of conference "Astrophysics in the Far Ultraviolet: Five Years of Discovery with FUSE", ASP Conf. Series (ed. Sonneborn, Moos, & Andersson)