Semiclassical approximation for low-degree stellar p modes - I. The classical eigenfrequency equation

Monthly Notices of the Royal Astronomical Society

Volumn 317, Issue 1, 2000, Pages 141-150

  Roxburgh, I W ^a   Vorontsov, S V ^b  

^a OBSERVATOIRE DE PARIS   (France)

^b SCHMIDT INSTITUTE OF PHYSICS OF THE EARTH   (Russian Federation)

Author keywords

Stars: oscillations; Waves Methods: numerical

Indexed keywords

ACOUSTIC WAVE PROPAGATION; NUMERICAL METHODS; STARS;

EIGENFREQUENCY; LOW DEGREE; METHOD: NUMERICAL; SEMI-CLASSICAL APPROXIMATION; SEMICLASSICAL APPROXIMATIONS; SOLAR LIKE OSCILLATIONS; STAR OSCILLATIONS; STELLAR P-MODES; WAVE - METHOD: NUMERICAL; WAVE METHOD;

ASYMPTOTIC ANALYSIS;

EID: 0000499916     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03623.x     Document Type: Article

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