Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..28..193m&link_type=abstract
Astrophysics and Space Science, Volume 28, Issue 1, pp.193-203
Astronomy and Astrophysics
Astrophysics
8
Scientific paper
Frequencies of non-radial oscillation of polytropic models of stars, belonging to spherical harmonics of ordersl=1, 2 and 3, are evaluated, in a ‘second approximation’, by a variational method. Equilibrium configurations in the presence of toroidal magnetic fields are obtained numerically without any restriction on the field strength. The value of the ratio of the specific heats, γ, is assumed to be equal to 5/3 and only two polytropic indeces,n=1.5 and 3.0, are considered. It is found that a polytropic star stays stable for magnetic fields considerably stronger than expected from the results obtained by the weak field perturbation methods.
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