Mn I hyperfine structure in the near-infrared
نویسندگان
چکیده
منابع مشابه
Mn i hyperfine structure in the near - infrared Jorge Meléndez ⋆
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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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1999
ISSN: 0035-8711,1365-2966
DOI: 10.1046/j.1365-8711.1999.02674.x