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Stably stratified stars containing magnetic fields whose toroidal components are much larger than the poloidal ones in general relativity: A perturbation analysis
Magnetic field strength at the innermost circular orbit in accretion disk of supermassive black hole in active galactic nuclei: comparison with the equipartition value
M. Y. Piotrovich, S. D. Buliga, Y. N. Gnedin, T. M. Natsvlishvili and N. A. Silant’ev Astrophysics and Space Science 357(2) (2015) https://doi.org/10.1007/s10509-015-2327-2
Formation of filament-like structures in the pulsar magnetosphere and the short-term variability of pulsar emission
MHD relaxation of fossil magnetic fields in stellar interiors
Stéphane Mathis, Vincent Duez and Jonathan Braithwaite Proceedings of the International Astronomical Union 6(S271) 270 (2010) https://doi.org/10.1017/S1743921311017698
ON THE STABILITY OF NON-FORCE-FREE MAGNETIC EQUILIBRIA IN STARS
A first model of stable magnetic configuration in stellar radiation zones
Vincent Duez, Jonathan Braithwaite and Stéphane Mathis Proceedings of the International Astronomical Union 6(S274) 467 (2010) https://doi.org/10.1017/S1743921311007514
Ideal instabilities in a high-β rotating cylindrical plasma in the presence of an azimuthal magnetic field and a gravitational field
A B Mikhailovskii, A M Fridman, A P Churikov, V D Pustovitov and A I Smolyakov Plasma Physics and Controlled Fusion 51(4) 045003 (2009) https://doi.org/10.1088/0741-3335/51/4/045003
Axisymmetric magnetic fields in stars: relative strengths of poloidal and toroidal components