Abstract
Of seven late K and early M dwarfs, six were observed to have magnetic fields. No relationship was seen between effective temperature and either field strength or filling factor. Magnetic flux was observed not to be constant over this range of effective temperature.
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References
Marcy, G.W. and Bruning, D.H. 1984, Ap. J. 281, 286.
Saar, S. 1987, Ap. J., in press.
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© 1987 Springer-Verlag
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Bruning, D.H., Chenoweth, R.E., Marcy, G.W. (1987). Magnetic fields on K and M dwarfs. In: Linsky, J.L., Stencel, R.E. (eds) Cool Stars, Stellar Systems, and the Sun. Lecture Notes in Physics, vol 291. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-18653-0_101
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DOI: https://doi.org/10.1007/3-540-18653-0_101
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