Mg II and Ca II emissions from three G dwarfs.
Bibcode: 1979A&A....76..249R
Rego, M.; Fernandez-Figueroa, M. J.
Spain
Abstract
The stars Eta Cet, Beta CnV, and Beta Com have been observed from the ground and the IUE satellite. The Ca II and Mg II K emission line intensities have been compared and show a correlation. The full widths at the base (FWB) corresponding to the Mg II K emission are in the dispersion band of the luminosity-FWB relationship.
1979
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Astronomy and Astrophysics
IUE
6