The autocorrelation function of stellar p-mode measurements and its diagnostic properties

Monthly Notices of the Royal Astronomical Society

Volumn 369, Issue 3, 2006, Pages 1491-1496

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

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b OBSERVATOIRE DE PARIS   (France)

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

Author keywords

Methods: numerical; Stars: oscillations

Indexed keywords

ACOUSTIC WAVE PROPAGATION; ACOUSTIC WAVES; AUTOCORRELATION; NUMERICAL METHODS; STARS;

AUTOCORRELATION FUNCTIONS; FREQUENCY SEPARATION; METHOD: NUMERICAL; P-MODE FREQUENCY; PHYSICAL QUANTITIES; PROPERTY; STAR OSCILLATIONS; STELLAR CORE; STELLAR INTERIOR; STELLAR P-MODES;

ACOUSTIC WAVE REFRACTION;

EID: 33745142190     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10396.x     Document Type: Article

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