Is the model of one-armed oscillations able to explain the long-termV/Rchanges of Be stars?
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20052727/pdf
Reference34 articles.
1. The envelopes of Be stars driven by optically thin lines
2. New grids of stellar models including tidal-evolution constants up to carbon burning
3. Effects of gravitational darkening on the determination of fundamental parameters in fast-rotating B-type stars
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3. HYDRODYNAMIC AND RADIATIVE MODELING OF TEMPORAL Hα EMISSIONV/RVARIATIONS CAUSED BY DISCONTINUOUS MASS TRANSFER IN BINARIES;The Astronomical Journal;2011-05-26
4. Properties and nature of Be stars;Astronomy & Astrophysics;2009-08-27
5. A PULSATIONAL MECHANISM FOR PRODUCING KEPLERIAN DISKS AROUND Be STARS;The Astrophysical Journal;2009-07-22
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