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- W2897801302 abstract "The absence of magnetic white dwarfs with a non-degenerate low-mass stellar companion in a wide binary is still very intriguing and at odds with the hypothesis that magnetic white dwarfs are the progenies of the magnetically peculiar Ap/Bp stars. On the other hand, we cannot resort to a process that impedes the generation of a strong magnetic field in the main or pre-main sequence progenitors of white dwarfs if they are in a multiple stellar system, because such a process would also prevent the formation of magnetic cataclysmic variables consisting of a magnetic white dwarf accreting mass from a low-mass companion. This is the reason why it has been proposed that fields in white dwarfs may be linked to their binarity and are generated through a dynamo mechanism during common envelope evolution." @default.
- W2897801302 created "2018-10-26" @default.
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- W2897801302 date "2018-10-15" @default.
- W2897801302 modified "2023-09-27" @default.
- W2897801302 title "The Origin of Magnetism in White Dwarfs" @default.
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