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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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sonraki gruplarýn üyesi:
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Kartal |
| Sað Açýklýk: | 19h39m18.96s |
| Yükselim: | +09°22'51.3" |
| Görünürdeki Parlaklýk: | 8.264 |
| özdevim Sað Açýklýk: | 53.3 |
| özdevim Yükselim: | -3.9 |
| B-T magnitude: | 9.142 |
| V-T magnitude: | 8.337 |
Kataloglar ve belirtme:
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