THE SPIN RATE OF PRE-COLLAPSE STELLAR CORES: WAVE-DRIVEN ANGULAR MOMENTUM TRANSPORT IN MASSIVE STARS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/810/i=2/a=101/pdf
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1. A New Class of Unstable Modes of Rotating Relativistic Stars
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3. TURBULENT CONVECTION IN STELLAR INTERIORS. II. THE VELOCITY FIELD
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5. Three-dimensional simulations of internal wave breaking and the fate of planets around solar-type stars
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