Mn I hyperfine structure in the near-infrared
Astrophysics
2009-10-31 v1 Atomic Physics
Abstract
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
Cite
@article{arxiv.astro-ph/9906180,
title = {Mn I hyperfine structure in the near-infrared},
author = {Jorge Melendez},
journal= {arXiv preprint arXiv:astro-ph/9906180},
year = {2009}
}
Comments
7 pages (including 9 figures). MNRAS (1999) accepted. PS version also available at http://www.iagusp.usp.br/~jorge/papers/hfsmnfinal.ps