Nazar Ikhsanov, Nina Beskrovnaya
Published 2014-01-21Version 1
Accretion-driven spin-up of a magnetized white dwarf in a close binary system is discussed. We address a situation in which the magnetic field of the white dwarf is screening during the accretion phase and re-generating due to the field diffusion through the accreted material after it. We find this scenario to be effective for a formation of massive pulsar-like white dwarfs.
Comments: 3 pages, to appear in Proc. of Thirteenth Marcel Grossmann Meeting - MG13
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