Fluorescence lines excited by the MG II resonance lines. II

Details Fluorescence lines excited by the MG II resonance lines. II Fluorescence lines excited by the MG II resonance lines. II

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....51..313g&link_type=abstract

Astronomy and Astrophysics, vol. 51, no. 2, Sept. 1976, p. 313-318.

Astronomy and Astrophysics

Astrophysics

2

Fluorescence, Line Spectra, Magnesium, Optical Resonance, Solar Spectra, Stellar Spectra, Chromosphere, Spectral Line Width, Spectral Resolution

Scientific paper

The influence of spectral resolution on the full width at the base of the emission core of the Mg II k line (2795.5 A) is determined by comparing solar observations with convolved profiles, and a width-magnitude relation is derived. The relation is used to predict the behavior of fluorescence lines excited by Mg II emission cores in Ke, Me, and N stars.

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