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Tom.Reding (talk | contribs) m →Magnetic cataclysmic variables: CS1 maint: Explicit use of et al. -> display-authors=etal using AWB |
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PG 1031+234 has a surface field that spans the range from ~200 MG to nearly 1000 MG and rotates with a period of 3<sup>h</sup>24<sup>m</sup>.<ref name=Latter>{{ cite journal |doi=10.1086/165543 |author=Latter WB |author2=Schmidt GD |author3=Green RF |title=The rotationally modulated Zeeman spectrum at nearly 10 to the 9th Gauss of the white dwarf PG 1031 + 234 |journal=Ap J. |date=1987 |volume=320 |pages=308 |bibcode=1987ApJ...320..308L}}</ref>
The magnetic fields in CVs are confined to a narrow range of strengths, with a maximum of 7080 MG for RX J1938.4-4623.<ref name=Schwope>{{ cite journal |title=Two-pole accretion in the high-field polar RXJ 1938.6-4612 |author=Schwope AD|
None of the single magnetic stars has been seen as of 1999 as an X-ray source, although fields are of direct relevance to the maintenance of coronae in main sequence stars.<ref name=Trimble/>
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