Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26as...64..477c&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 64, no. 3, June 1986, p. 477-486.
Astronomy and Astrophysics
Astrophysics
7
A Stars, Abundance, Giant Stars, Hertzsprung-Russell Diagram, Peculiar Stars, Spectral Line Width, Stellar Spectra, Astronomical Catalogs, Spectrum Analysis
Scientific paper
The present 3800-6700 A line identifications and equivalent widths for the Am star HR 178 were produced by a reduction procedure that used a Fourier transform analysis to suppress high frequencies that are due to photographic emulsion noise. In order to eliminate systematic instrumental effects between these spectra and those of 15 Vul, spectra are also obtained for this star using the same methods. It is found that the best agreements exist among the different abundance determinations for each element from neutral and ionized stages, in both absolute and differential growth curves, for the blue and red spectral ranges.
Burkhart C.
Coupry M. F.
van't Veer-Menneret C.
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