Coordinated UV and X-Ray Spectroscopic Observations of the O-type Giant ξ Per: The Connection between X-Rays and Large-scale Wind Structure
Author:
Funder
NASA/HST GO program
Deutsches Zentrum fur Luft und Raumfahrt
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/873/i=1/a=81/pdf
Reference55 articles.
1. Radiation-driven winds in Of stars
2. Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive
3. Hydrodynamical Simulations of Corotating Interaction Regions and Discrete Absorption Components in Rotating O-Star Winds
4. Investigating the origin of cyclical wind variability in hot, massive stars – I. On the dipolar magnetic field hypothesis★
5. A search for the cause of cyclical wind variability in O stars
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