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• W3100925531 abstract "Context. Most planetary nebulae have bipolar or other non-spherically symmetric shapes. Magnetic fields in the central star may be responsible for this lack of symmetry, but observational studies published to date have reported contradictory results." @default.
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• W3100925531 date "2012-06-01" @default.
• W3100925531 modified "2023-09-30" @default.
• W3100925531 title "Magnetic fields in central stars of planetary nebulae?" @default.
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• W3100925531 doi "https://doi.org/10.1051/0004-6361/201219175" @default.
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