Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.132...85s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 132, no. 1, April 1987, p. 85-104. UGCI-supported research.
Astronomy and Astrophysics
Astrophysics
3
Magnetic Field Configurations, Stellar Magnetic Fields, Stellar Mass, Stellar Oscillations, Stellar Structure, Stellar Models, Vibration Mode
Scientific paper
The equilibrium structure and oscillations of a partially degenerate standard model in the presence of a poloidal magnetic field have been studied. The magnetic field in the interior has been matched with an outside dipole field. The effect of magnetic field on the various structural parameters, e.g., mass, central condensation, moment of inertia, and oblateness has been computed for different values of the central degeneracy of the model. The effect of magnetic field on radial oscillations of the configuration is also studied. A variational formulation is used to compute the changes in the frequency of radial mode of oscillation. It has been shown that the changes in frequency computed for various models using a two-parameter eigenfunction are in fair agreement with the values obtained by using the exact eigenfunction.
Das Mrinal K.
Pal Singh Harinder
Tandon J. N.
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