A criterion of double-mode pulsation from coupling coefficients

Details A criterion of double-mode pulsation from coupling coefficients A criterion of double-mode pulsation from coupling coefficients

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.167..173i&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 167, no. 1, May 1990, p. 173-176.

Astronomy and Astrophysics

Astrophysics

2

Cepheid Variables, Pulsars, Stellar Oscillations, Coupled Modes, Stellar Evolution, Stellar Models

Scientific paper

A criterion for the occurrence of double-mode pulsations is derived from
linear adiabatic coupling coefficients. The criterion indicates that
double-mode pulsations of classical Cepheids occur at a shorter period
range than the observed one, and that the evolutionary mass models are
preferable for the double-mode pulsations.

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