Stellar disharmony

Details Stellar disharmony Stellar disharmony

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.235..875c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 235, Dec. 15, 1988, p. 875-880. Research supported by t

Computer Science

Sound

25

Asymptotic Methods, Stellar Models, Stellar Oscillations, Stellar Structure, Acoustic Velocity, Frequency Distribution

Scientific paper

Frequency differences between high-order p-modes of two stellar models, both with the mass and luminosity of the sun, are compared with results of asymptotic theory. The computed relative differences are closely approximated by averages of the relative sound-speed differences, weighted by the local sound travel-time, over the regions where the modes are trapped.

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