A note on a property of pulsating stars

Details A note on a property of pulsating stars A note on a property of pulsating stars

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.132...53k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 132, no. 1, April 1987, p. 53-56.

Statistics

Computation

1

Cepheid Variables, Stellar Oscillations, Stellar Physics, Boundary Value Problems, Computational Astrophysics, Stellar Atmospheres, Thermodynamics

Scientific paper

An explanation for the observed correlation between the ratio (relative amplitude of flux variation)/(relative amplitude of radius variation) and the period of radial pulsation in cepheids is proposed. If the explanation is correct, correlations may be expected for other classes of pulsating stars with the general functional form determined by physical conditions in the atmosphere.

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