A Clue to the Extent of Convective Mixing Inside Massive Stars: The Surface Hydrogen Abundances of Luminous Blue Variables and Hydrogen‐poor Wolf‐Rayet Stars-Reference-Cited by-同舟云学术

A Clue to the Extent of Convective Mixing Inside Massive Stars: The Surface Hydrogen Abundances of Luminous Blue Variables and Hydrogen‐poor Wolf‐Rayet Stars

Published:2000-09-10 Issue:2 Volume:540 Page:1041-1048
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Stothers Richard B.,Chin Chao‐wen

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/540/i=2/a=1041/pdf

Reference84 articles.

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2. The evolution of massive stars with mass loss

3. Theoretical models for massive stars in young Magellanic Cloud stellar clusters

4. Turbulence in Stars. III. Unified Treatment of Diffusion, Convection, Semiconvection, Salt Fingers, and Differential Rotation

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