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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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Not Available
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Observation and Astrometry data
| Constellation: | Αετός |
| Right ascension: | 19h14m32.54s |
| Declination: | +10°33'19.0" |
| Apparent magnitude: | 8.258 |
| Distance: | 3571.429 parsecs |
| Proper motion RA: | 1.2 |
| Proper motion Dec: | 2.2 |
| B-T magnitude: | 8.759 |
| V-T magnitude: | 8.3 |
Catalogs and designations:
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