Open AccessMn i hyperfine structure in the near‐infrared
Author(s) -
Meléndez Jorge
Publication year - 1999
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.1999.02674.x
Subject(s) - hyperfine structure , physics , infrared , line (geometry) , astrophysics , absorption (acoustics) , absorption spectroscopy , atomic physics , spectral line , infrared spectroscopy , astronomy , optics , geometry , mathematics , quantum mechanics
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.