Physics
Scientific paper
Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pomic..12...23b&link_type=abstract
Publ. Obs. Univ. Michigan, Vol. 12, No. 2, p. 23 - 75
Physics
2
Abundance, Characterization, Magnetic Stars, Wavelengths, Fine Structure, Line Spectra, Tables (Data)
Scientific paper
The unusually sharp spectral lines of HR 4816 make it particularly well suited for identification work at high dispersion. The 2A/mm spectrogram (EC 103) was taken at the Lick Observatory. The UT data of mid-exposure was 7.26 June 1960, (2437092.76). The bulk of the identifications were made in 1960, from wavelengths measured with a conventional engine. In the list, the stellar wavelengths are in the first column, followed by an estimate of the intensity and character of the line, the identifications begin in column 4 with decimal fractions of an angstrom. The multiplet number follows the symbol for the atomic spectrum.
Bidelman Wiliam P.
Cowley Charles R.
Roemmelt John C.
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