Wave Heating and Range of Stellar Activity in Late-Type Dwarfs

Details Wave Heating and Range of Stellar Activity in Late-Type Dwarfs Wave Heating and Range of Stellar Activity in Late-Type Dwarfs

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001apj...559l.167u&link_type=abstract

The Astrophysical Journal, Volume 559, Issue 2, pp. L167-L170.

Astronomy and Astrophysics

Astronomy

18

Stars: Activity, Stars: Chromospheres

Scientific paper

Theoretical time-dependent and two-component chromospheric models for late-type dwarfs are constructed based on acoustic and magnetic wave heating mechanisms. The models are used to predict the theoretical range of chromospheric activity for these stars. Comparison of this range with the one established observationally shows that the wave heating alone can explain most but not all of the observed range of stellar activity.

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