A conjecture regarding the dMe stars

Details A conjecture regarding the dMe stars A conjecture regarding the dMe stars

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974pasp...86..595w&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 86, Oct. 1974, p. 595-598.

Astronomy and Astrophysics

Astronomy

13

Late Stars, M Stars, Main Sequence Stars, Stellar Atmospheres, Stellar Magnetic Fields, Electric Fields, Magnetic Flux, Solar Magnetic Field, Stellar Spectra, Surface Properties, Variable Stars

Scientific paper

The dMe stars are late-type main-sequence objects which exhibit characteristics that can be explained as the result of solar-type surface magnetic activity. The battery mechanism of Biermann (1950) is used to explain the origin of the magnetic fields responsible for the surface activity. Magnetic fields 10-100 times the strength of solar magnetic fields can be produced in this manner. Such strong fields are consistent with the observed dMe properties and should be directly detectable.

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