A semi-analytical formula for the light variations due to low-frequency g modes in rotating stars

Monthly Notices of the Royal Astronomical Society

Volumn 343, Issue 1, 2003, Pages 125-136

  Townsend, R H D ^a  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

Author keywords

Methods: analytical; Stars: oscillations; Stars: rotation; Techniques: photometric

Indexed keywords

PHOTOMETRY; ROTATION; WAVEGUIDES;

G-MODES; LOWER FREQUENCIES; METHODS:ANALYTICAL; ROTATING STARS; SEMI-ANALYTICAL FORMULAE; STAR OSCILLATIONS; STARS: ROTATION; STELLAR MODELING; TECHNIQUES: PHOTOMETRIC; TRADITIONAL APPROXIMATION;

STARS;

EID: 0142118283     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06640.x     Document Type: Article

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