Abstract
Expressions for the amplitudes and phases of the light, colour and radial velocity variations are derived for a star in nonradial oscillation. For stars in the cepheid instability strip the spherical harmonic mode of the oscillation can be obtained from the phase difference between the light and colour variations. For β Cep stars the mode can be estimated from the amplitude ratio of the light and colour variations.
Similar content being viewed by others
Reference
Balona, L.A., 1981. Mon. Not. R. astr. Soc., in press.
Balona, L.A. & Stobie, R.S., 1979a. Mon. Not. R. astr. Soc., 187, pp. 217–22.
Balona, L.A. & Stobie, R.S., 1979b. Mon. Not. R. astr. Soc., 189, pp. 649–58.
Balona, L.A. & Stobie, R.S., 1980. Mon. Not. R. astr. Soc., 190, pp 931–43.
Balona, L.A., Dean, J.F. & Stobie, R.S., 1980. Mon. Not. R. astr. Soc., in press.
Dziembowski, W., 1977. Acta Astronomica, 27, pp. 203–11.
Kurtz, D.W., 1980a. Mon. Not. R. astr. Soc., 191, pp. 115–22.
Kurtz, D.W., 1980b. Mon. Not. R. astr. Soc., in press.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Balona, L.A., Stobie, R.S. Mode discrimination in nonradially oscillating stars from light, colour and velocity observations. Space Sci Rev 27, 371–376 (1980). https://doi.org/10.1007/BF00168322
Issue Date:
DOI: https://doi.org/10.1007/BF00168322