Mn i hyperfine structure in the near - infrared Jorge Meléndez ⋆
نویسنده
چکیده
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-˚ A solar absorption line as resulting from Mn i, and I discarded the identifications of the 13281.65-˚ A and 16929.85-˚ A solar features as a result of Fe i and Mn i, respectively.
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