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Asteroseismology of the SPB star HD 21071
Published online by Cambridge University Press: 23 January 2015
Abstract
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We perform mode identification for the frequency peaks detected in the light variation of HD 21071 including the effects of rotation via the traditional approximation. We find the angular numbers (ℓ, m) for all observed frequencies and limit the range of the rotational velocity. In the next step, we make an attempt towards seismic modelling of the star in order to constrain its global parameters.
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- Copyright © International Astronomical Union 2015
References
Daszyńska-Daszkiewicz, J., Dziembowski, W. A., & Pamyatnykh, A. A. 2008, Journal of Physics Conference Series 118 (1), 012024CrossRefGoogle Scholar
De Cat, P. 2002, in IAU Colloq. 185: Radial and Nonradial Pulsationsn as Probes of Stellar Physics, Vol. 259 of Astronomical Society of the Pacific Conference Series, p. 196Google Scholar
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