Mn I hyperfine structure in the near-infrared

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

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

Cited by in corpus (6)

• Oscillator Strengths and Damping Constants for Atomic Lines in the J and H Bands
• Keck-Nirspec Infrared OH Lines: Oxygen Abundances in Metal-Poor Stars Down to [Fe/H] = -2.9
• Oxygen Abundances in Metal-Poor Stars (-2.2 < [Fe/H] < -1.2) from Infrared OH lines
• Spectral analysis of high resolution near-infrared spectra of ultra cool dwarfs
• Hyperfine dependent $gf$-values of Mn I lines in the 1.49 $-$ 1.80 $\mu$m H-band
• Hyperfine splitting of [Al VI]3.66um and the Al isotopic ratio in NGC6302