Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pasp..101..681a&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, July 1989, p. 681-683. Research supported by the C
Astronomy and Astrophysics
Astrophysics
3
Astronomical Spectroscopy, High Dispersion Spectrographs, Photographic Plates, Stellar Spectra, Data Processing, Metallicity, Signal To Noise Ratios, Spectral Line Width
Scientific paper
High-dispersion 2.4 A/mm spectra with signal-to-noise ratios of order 80 were obtained for three stars by using a Reticon detector and by coadding photographic spectrograms at the Dominion Astrophysical Observatory. Metal lines of equivalent widths 5 to 75 mA in Alpha Dra and Iota CrB show systematic differences of order 4 percent with an uncertainty of order 3 percent and an rms scatter of 2.0 to 3.7 mA about the mean equivalent-width differences.
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