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Mn i hyperfine structure in the near-infrared
Authors:Jorge Meléndez
Institution:Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT
Abstract:Hyperfine interaction constants and hyperfine components of Mn  i lines in the near-infrared J and H bands were obtained by fitting the solar spectrum. I identified the 17744-Å solar absorption line as resulting from Mn  i , and I discarded the identifications of the 13281.65-Å and 16929.85-Å solar features as a result of Fe  i and Mn  i , respectively.
Keywords:stars: individual: κ vel  turbulence  ISM: atoms    ISM: clouds    ISM: structure
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