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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
Element spots in Ap and Hg‐Mn stars from current‐driven diffusion
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
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
Axisymmetric magnetic fields in stars: relative strengths of poloidal and toroidal components
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
Current‐driven instabilities in weakly ionized disks