Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26as...26...89b&link_type=abstract
Astronomy and Astrophysics Supplement Series, vol. 26, Oct. 1976, p. 89-128. Research supported by the Fonds de la Recherche Fo
Astronomy and Astrophysics
Astrophysics
18
Infrared Spectra, Solar Spectra, Spectral Line Width, Spectrum Analysis, Transition Metals, Chromium, Cobalt, Iron, Manganese, Nickel, Scandium, Titanium, Vanadium
Scientific paper
By using theoretical oscillator strengths recently obtained by Kurucz and Peytremann (1975), solar equivalent widths have been calculated for approximately 20,000 infrared lines of the iron-group elements in the wavelength range from 1 to 10 microns. The results have been compared with observed profiles measured on the most recent solar spectra. From these comparisons, 200 new identifications are proposed, and many previous ones are confirmed.
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