Line identifications in the spectrum of HR 1100

Details Line identifications in the spectrum of HR 1100 Line identifications in the spectrum of HR 1100

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..979m&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 94, Dec. 1982, p. 979-986. Research supported by the Comision de Investi

Other

Abundance, Astronomical Catalogs, Line Spectra, Peculiar Stars, Spectrum Analysis, Stellar Spectra, Atomic Spectra, Doppler Effect, Iron, Manganese, Potassium, Radial Velocity, Silicon, Stellar Spectrophotometry, Titanium, Wavelengths

Scientific paper

The spectrum of the star HR 1100 has been studied. The atomic species
present on two coude spectrograms of the star are identified. Fe is
found in the first three stages of ionization, Si II, Si III, P II, P
III, Ti II, Ti III, Mn II, Hg II, and Sr II, among others. The results
for HR 1100 are compared with the results for other anomalous objects.

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