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Title
What controls the magnetic geometry of M dwarfs?
Authors
Keywords
-
Journal
ASTRONOMY & ASTROPHYSICS
Volume 549, Issue -, Pages L5
Publisher
EDP Sciences
Online
2012-12-06
DOI
10.1051/0004-6361/201220317
References
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Related references
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- Large-scale magnetic topologies of late M dwarfs★
- (2010) J. Morin et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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- (2009) J.-F. Donati et al. Annual Review of Astronomy and Astrophysics
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- EVIDENCE FOR MAGNETIC FLUX SATURATION IN RAPIDLY ROTATING M STARS
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- (2009) R. D. Simitev et al. EPL
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- (2009) A. Cattaneo et al. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Energy flux determines magnetic field strength of planets and stars
- (2009) Ulrich R. Christensen et al. NATURE
- Dynamo Scaling Laws and Applications to the Planets
- (2009) U. R. Christensen SPACE SCIENCE REVIEWS
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- (2008) Matthew K. Browning ASTROPHYSICAL JOURNAL
- Relations between the dynamo region geometry and the magnetic behavior of stars and planets
- (2008) L. Goudard et al. EPL
- Large-scale magnetic topologies of mid M dwarfs★
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- The stable magnetic field of the fully convective star V374 Peg
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