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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: | へびつかい座 |
| Right ascension: | 17h26m39.96s |
| Declination: | -01°00'06.0" |
| Apparent magnitude: | 7.645 |
| Distance: | 147.929 parsecs |
| Proper motion RA: | 16.6 |
| Proper motion Dec: | -17 |
| B-T magnitude: | 8.034 |
| V-T magnitude: | 7.678 |
Catalogs and designations:
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