Relating turbulent pressure and macroturbulence across the HR diagram with a possible link toγDoradus stars
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201527289/pdf
Reference37 articles.
1. Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars
2. THE ROLE OF TURBULENT PRESSURE AS A COHERENT PULSATIONAL DRIVING MECHANISM: THE CASE OF THE δ SCUTI STAR HD 187547
3. Connections Between Stellar Oscillations and Turbulent Convection
4. Theoretical seismic properties of pre-main sequenceγ Doradus pulsators
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