Metal abundances of F and G dwarfs determined by the radial velocity scanner CORAVEL

Details Metal abundances of F and G dwarfs determined by the radial velocity scanner CORAVEL Metal abundances of F and G dwarfs determined by the radial velocity scanner CORAVEL

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....87l...1m&link_type=abstract

Astronomy and Astrophysics, vol. 87, no. 1-2, July 1980, p. L1, L2.

Astronomy and Astrophysics

Astrophysics

56

Abundance, Dwarf Stars, F Stars, G Stars, Iron, Metallic Stars, Stellar Spectra, Chemical Composition, Interstellar Extinction, Optical Scanners, Radial Velocity, Stellar Rotation

Scientific paper

A new method for determining [Fe/H] is proposed. The study of a sample of F and G dwarfs with [Fe/H] determined homogeneously at high dispersion shows that the precision of this new method is equivalent to the best existing methods. Moreover, it presents numerous advantages, in particular its rapidity, sensitivity and independence with respect to interstellar reddening.

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