Abstract:There are no known examples of magnetic white dwarfs with fields larger than ∼ 3 MG paired with a non-degenerate companion in detached binary systems. The suggestion is that highly magnetic, isolated white dwarfs may originate from stars that coalesce during common envelope evolution while those stars that emerge from a common envelope on a close orbit may evolve into double degenerate systems consisting of two white dwarfs, one or both magnetic.The presence of planets or planetary debris around white dwarfs i… Show more
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