Stellar metallicity gradient in the direction of the south galactic pole determined from Walraven photometry

Details Stellar metallicity gradient in the direction of the south galactic pole determined from Walraven photometry Stellar metallicity gradient in the direction of the south galactic pole determined from Walraven photometry

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984msngr..35...32t&link_type=abstract

ESO Messenger (ISSN 0722-6691), March 1984, p. 32-35.

Physics

Metallicity, Milky Way Galaxy, Star Distribution, Stellar Spectrophotometry, Ubv Spectra, Calibrating, Distance, Galactic Evolution, Stellar Gravitation, Stellar Temperature

Scientific paper

The observations presently reported were aimed at determining the relation between stellar metal abundance and distance from the galactic plane in a wider solar neighborhood. The Basel RGU Survey is used for the selection of F- and G-type program stars, thereby extending earlier photoelectric work to greater distances. A semiempirical calibration of the (V-B)-(B-L) diagram is constructed by combining the theoretical Kurucz colors with observations of field stars that cover a wide metallicity range.

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