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Cited article:

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Discovery and analysis of three magnetic hot subdwarf stars: evidence for merger-induced magnetic fields

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Single magnetic white dwarfs with Balmer emission lines: a small class with consistent physical characteristics as possible signposts for close-in planetary companions

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Where are the double-degenerate progenitors of Type Ia supernovae?

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The violent white dwarf merger scenario for the progenitors of Type Ia supernovae

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New binaries among UV-selected, hot subdwarf stars and population properties★

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Orbital solutions of eight close sdB binaries and constraints on the nature of the unseen companions

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