Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993japa...14..145p&link_type=abstract
Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 14, no. 3-4, p. 145-165
Astronomy and Astrophysics
Astrophysics
21
Abundance, Metallicity, Red Giant Stars, Stellar Color, Stellar Composition, Stellar Spectrophotometry, Color-Color Diagram, Cyanogen, High Dispersion Spectrographs, Iterative Solution, Solar Neighborhood, Ubv Spectra
Scientific paper
Several arguments that justify establishing a revised abundance calibration for DDO photometry of population I red giants are presented. The components of the blanketing vector in the DDO C(45-48) vs C(42-45) diagram are determined for late-type dwarfs and giants. We have redefined the DDO cyanogen anomaly and calibrated it against metallicity. The sample of field giants now available with abundances derived from high dispersion spectroscopy is substantially larger than previously available, leading to a more accurate abundance calibration. Iso-abundance lines in the C(41-42) vs C(42-45) diagram have been determined for population IG and K giants and an iterative method for deriving abundances of these stars is described. We show that the new DDO abundances are in very good agreement with those derived from high dispersion spectroscopy. The new method improves by about 0.1 dex the DDO abundances derived for early G and/or late K giants, with respect to the delta(CN) method of Janes (1975).
Claria Juan J.
Piatti Andrés E.
~Minniti Dante
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