Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...149..167h&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 149, no. 1, Aug. 1985, p. 167-170.
Astronomy and Astrophysics
Astrophysics
15
Abundance, Stellar Atmospheres, Stellar Composition, A Stars, Atmospheric Composition, Iron, Metallicity, Stellar Spectra
Scientific paper
Abundance analysis results of the δ Del star 20 CVn are reported. The following atmospheric parameters are derived: θeff = 0.70, log g = 3.0, [Fe/H]_sun;20 CVn = +0.48, ξ = 0.9 km s-1. The high iron abundance fits the large value of Δm2, the blanketing parameter in the Geneva photometric system. This result tends to confirm that it is possible to use Δm2 to study the metallicity in the atmosphere of δ Del stars.
Foy Renaud
Hauck B.
Proust Dominique
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