Width-luminosity relationship of the MG II K line in late-type stars

Details Width-luminosity relationship of the MG II K line in late-type stars Width-luminosity relationship of the MG II K line in late-type stars

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...204..147e&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 204, no. 1-2, Oct. 1988, p. 147, 148.

Astronomy and Astrophysics

Astrophysics

11

Late Stars, Metallicity, Stellar Luminosity, Stellar Spectra, Chromosphere, Magnesium

Scientific paper

The linear relationship found between the width of the Mg II k line and the luminosity of late-type stars is shown to be valid over a range of 17 mag in luminosity. Results suggest that this relationship may also be valid in the region of red dwarfs. It is noted that this width-luminosity relationship can be extended into the region of stars of low luminosity for other chromospheric lines.

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