Astronomy and Astrophysics – Astronomy
Scientific paper
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.
Fawzy Diaa
Musielak Zdzislaw E.
Stepien Kazimierz
Ulmschneider Peter
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