A comparison of the MG resonance lines in AM and non AM stars of similar temperatures

Details A comparison of the MG resonance lines in AM and non AM stars of similar temperatures A comparison of the MG resonance lines in AM and non AM stars of similar temperatures

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....92..219b&link_type=abstract

Astronomy and Astrophysics, vol. 92, no. 1-2, Dec. 1980, p. 219-221.

Astronomy and Astrophysics

Astrophysics

5

A Stars, Line Spectra, Magnesium, Optical Resonance, Stellar Spectra, Ultraviolet Spectra, Absorption Spectra, H Lines, K Lines, Stellar Rotation, Stellar Temperature

Scientific paper

A comparison of the Mg II resonance lines in Am and none Am stars of
similar effective temperatures does not show any measurable
differences. The Mg I resonance lines may be weaker in the Am
stars. The mechanism reducing the Ca II K line intensities in Am stars
does not work for the Mg II k and h lines.

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