MG II and CA II emissions from three G dwarfs

Details MG II and CA II emissions from three G dwarfs MG II and CA II emissions from three G dwarfs

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....76..249r&link_type=abstract

Astronomy and Astrophysics, vol. 76, no. 2, July 1979, p. 249-251.

Astronomy and Astrophysics

Astronomy

6

Astronomical Spectroscopy, Calcium, Dwarf Stars, G Stars, Manganese, Metal Ions, Emission Spectra, Iue, K Lines, Spaceborne Astronomy, Width

Scientific paper

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.

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