Mn I hyperfine structure in the near-infrared

Details Mn I hyperfine structure in the near-infrared Mn I hyperfine structure in the near-infrared

1999-06-10

arxiv.org/abs/astro-ph/9906180v1

Mon.Not.Roy.Astron.Soc. 307 (1999) 197

Astronomy and Astrophysics

Astrophysics

7 pages (including 9 figures). MNRAS (1999) accepted. PS version also available at http://www.iagusp.usp.br/~jorge/papers/hfsm

Scientific paper

10.1046/j.1365-8711.1999.02674.x

Hyperfine interaction constants and hyperfine components of MnI lines in the
near-infrared J and H bands were obtained by fitting the solar spectrum. I
identified the 17744-A solar absorption line as resulting from MnI and I
discarded the identifications of the 13281.65-A and 16929.85-A solar features
as a result of FeI and MnI, respectively

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