Stroemgren photometry of F- and G-type stars brighter than V = 9.6. I. UVBY photometry

Details Stroemgren photometry of F- and G-type stars brighter than V = 9.6. I. UVBY photometry Stroemgren photometry of F- and G-type stars brighter than V = 9.6. I. UVBY photometry

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26as..106..257o&link_type=abstract

Astronomy and Astrophysics Suppl. 106, 257-266 (1994)

Astronomy and Astrophysics

Astrophysics

107

Galaxy: Solar Neighbourhood, Stellar Content, Stars: Late Type, Fundamental Parameters, Catalogues

Scientific paper

Within the framework of a large photometric observing program, designed to investigate the Galaxy's structure and evolution, Hβ photometry is being made for about 9000 stars. As a by-product, supplementary uvby photometry has been made. The results are presented in a catalogue containing 6924 uvby observations of 6190 stars, all south of δ=+38deg. The overall internal rms errors of one observation (transformed to the standard system) of a program star in the interval 6.5

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