Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.117..381m&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 117, no. 2, Dec. 1985, p. 381-385.
Astronomy and Astrophysics
Astrophysics
4
Chromosphere, Dwarf Stars, H Alpha Line, Stellar Activity, Stellar Rotation, Emission Spectra, Late Stars, Stellar Spectra
Scientific paper
The dependence of H-alpha emission strength on rotational period and spectral type in late-type stars is studied using published data. The emission strength shows strong correlation with rotation irrespective of age and spectral type. The chromospheric H-alpha emission strength in late-type dwarfs is a good diagnostic of rotation period in accordance with dynamo theory.
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