Asteroseismology of the SPB star HD 21071

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...

Full description

Saved in:
Bibliographic Details
Published in:Proceedings of the International Astronomical Union 2014-06, Vol.9 (S307), p.232-234
Main Authors: Szewczuk, Wojciech, Daszyńska-Daszkiewicz, Jadwiga
Format: Article
Language:English
Subjects:
Angular velocity
Approximation
Astronomical bodies
Astronomical instruments
Astronomy
Astrophysics
Contributed Papers
Mathematical analysis
Mathematical models
Rotation
Stars
Stars & galaxies
Citations: Items that this one cites
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary: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.
ISSN:1743-9213
1743-9221
DOI:10.1017/S174392131400684X