On the possibility of resonant electrodynamic coupling in the coronae of red dwarfs

Details On the possibility of resonant electrodynamic coupling in the coronae of red dwarfs On the possibility of resonant electrodynamic coupling in the coronae of red dwarfs

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...282..603m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 282, July 15, 1984, p. 603-611.

Astronomy and Astrophysics

Astrophysics

42

Red Dwarf Stars, Stellar Coronas, Stellar Temperature, X Ray Sources, Convection, Coupling, M Stars, Solar Atmosphere

Scientific paper

The authors suggest that, in the context of Ionson's electrodynamic coupling theory of coronal heating, the coupling efficiency may pass through a resonance in lower main-sequence stars. It is proposed that this resonance contributes to the strong observed X-ray emission in early-M dwarfs. In the coolest M dwarfs, the efficiency is expected to decrease rapidly as conditions move away from resonance.

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