Effect of rotational mixing and metallicity on the hot star wind mass-loss rates-Reference-Cited by-同舟云学术

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Effect of rotational mixing and metallicity on the hot star wind mass-loss rates

Published:2014-07 Issue: Volume:567 Page:A63
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Krtička J.,Kubát J.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201423845/pdf

Reference34 articles.

1. The theory of radiatively driven stellar winds. II - The line acceleration

2. The Chemical Composition of the Sun

3. The Ofpe/WN9 Stars in M33

4. Massive stars at low metallicity

5. Grids of stellar models with rotation

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1. Massive stars in extremely metal-poor galaxies: a window into the past;Experimental Astronomy;2021-06

2. Overstable convective modes in rotating early-type stars;Monthly Notices of the Royal Astronomical Society;2021-05-22

3. Hot subdwarf wind models with accurate abundances;Astronomy & Astrophysics;2019-10-22

4. Low-metallicity massive single stars with rotation;Astronomy & Astrophysics;2019-02-25

5. Hot star wind mass-loss rate predictions at low metallicity;Proceedings of the International Astronomical Union;2018-08

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