Equilibrium structure of stars with radiation pressure in the presence of a magnetic field

Details Equilibrium structure of stars with radiation pressure in the presence of a magnetic field Equilibrium structure of stars with radiation pressure in the presence of a magnetic field

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72..397d&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 2, Oct. 1980, p. 397-410. Research supported by the Indian National Science Academ

Astronomy and Astrophysics

Astrophysics

1

Main Sequence Stars, Radiation Pressure, Stellar Magnetic Fields, Stellar Structure, Equilibrium Equations, Perturbation Theory, Pressure Effects, Stellar Models, Tensors

Scientific paper

Equilibrium configuration of the upper Main-Sequence stars, with significant radiation pressure and having an interior magnetic field (matching with an external dipole field) has been considered. The structural parameters have been calculated for low and high magnetic fields by using a first-order perturbation method and a modified perturbation technique respectively. With the increase of radiation pressure, the star is seen to become more centrally condensed

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