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Stroemgren photometry of F- and G-type stars brighter than V = 9.6. I. UVBY photometry Within the framework of a large photometric observing program, designedto investigate the Galaxy's structure and evolution, Hβ photometryis being made for about 9000 stars. As a by-product, supplementary uvbyphotometry has been made. The results are presented in a cataloguecontaining 6924 uvby observations of 6190 stars, all south ofδ=+38deg. The overall internal rms errors of one observation(transformed to the standard system) of a program star in the interval6.5
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Observation and Astrometry data
Constellation: | Αετός |
Right ascension: | 19h32m26.79s |
Declination: | +09°35'47.5" |
Apparent magnitude: | 8.498 |
Proper motion RA: | 17.2 |
Proper motion Dec: | 9.5 |
B-T magnitude: | 8.841 |
V-T magnitude: | 8.527 |
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