Helium Star Models with Optically Thick Winds: Implications for the Internal Structures and Mass-loss Rates of Wolf–Rayet Stars
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/852/i=2/a=126/pdf
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1. A higher-than-predicted measurement of iron opacity at solar interior temperatures
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1. The temperature dependency of Wolf–Rayet-type mass loss;Astronomy & Astrophysics;2023-02
2. The Wolf–Rayet Stellar Response To The Iron Opacity Bump: Envelope Inflation, Winds, and Microturbulence;The Astrophysical Journal;2019-03-06
3. The Galactic WC and WO stars;Astronomy & Astrophysics;2019-01
4. Subsonic structure and optically thick winds from Wolf–Rayet stars;Astronomy & Astrophysics;2018-06
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