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Polarized Radiation from White Dwarfs and Atoms in Strong Magnetic Fields
Symposium - International astronomical union
We present the recent results of our continuing program of investigation of the behavior of matter in strong to super-strong magnetic fields (B∼ 106−1012G). This work was motivated by the discovery of strong magnetic fields (B∼ 107G) in some white dwarfs and the likely existence of super-strong fields (B∼ 1012G) in pulsars. Magnetic white dwarfs were discovered from observations of the continuous spectrum and one of the most intriguing challenges for the theorist is to provide an explanationdoi:10.1017/s0074180900100087 fatcat:vt5apzvxlzglplos76cyfgl6da