Stability of g modes in rotating B-type stars
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/412/4/2265/3335170/mnras0412-2265.pdf
Reference23 articles.
1. Gravity modes in rapidly rotating stars
2. MOSTDetects SPBe Pulsations in HD 127756 and HD 217543: Asteroseismic Rotation Rates Independent ofv sin i
3. The nonadiabatic analysis of nonradial modes of stellar oscillation in the presence of slow rotation
4. Observational Asteroseismology of slowly pulsating B stars
5. The opacity mechanism in B-type stars - II. Excitation of high-order g-modes in main-sequence stars
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1. Non-linear three-mode coupling of gravity modes in rotating slowly pulsating B stars;Astronomy & Astrophysics;2024-07
2. Domains of pulsational instability of low-frequency modes in rotating upper main sequence stars;Monthly Notices of the Royal Astronomical Society;2017-05-06
3. Period–luminosity relations of fast-rotating B-type stars in the young open cluster NGC 3766;Monthly Notices of the Royal Astronomical Society;2017-02-11
4. SUB-INERTIAL GRAVITY MODES IN THE B8V STAR KIC 7760680 REVEAL MODERATE CORE OVERSHOOTING AND LOW VERTICAL DIFFUSIVE MIXING;The Astrophysical Journal;2016-05-31
5. Pulsation-driven mean zonal and meridional flows in rotating massive stars;Monthly Notices of the Royal Astronomical Society;2016-02-10
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