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Does GD 356 have a terrestrial planetary companion?

Wickramasinghe, Dayal; Farihi, Jay; Tout, Christopher A; Ferrario, Lilia; Stancliffe, Richard J

Description

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

CollectionsANU Research Publications
Date published: 2010
Type: Journal article
URI: http://hdl.handle.net/1885/53707
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1111/j.1365-2966.2010.16417.x

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