Does GD 356 have a terrestrial planetary companion?
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Date
Authors
Wickramasinghe, Dayal
Farihi, Jay
Tout, Christopher A
Ferrario, Lilia
Stancliffe, Richard J
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Volume Title
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Blackwell Publishing Ltd
Abstract
GD 356 is unique among magnetic white dwarfs because it shows Zeeman-split Balmer lines in pure emission. The lines originate from a region of nearly uniform field strength (δB/B≈ 0.1) that covers 10 per cent of the stellar surface in which there is a
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Monthly Notices of the Royal Astronomical Society
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Book Title
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Restricted until
2037-12-31