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arXiv · 1401.5374

Formation and appearance of pulsar-like white dwarfs

Nazar Ikhsanov·Nina Beskrovnaya
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Abstract

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.

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Nazar Ikhsanov, Nina Beskrovnaya. 2014-01-21. Formation and appearance of pulsar-like white dwarfs. https://doi.org/10.1142/9789814623995_0467

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