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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: | Koc |
| Sað Açýklýk: | 02h53m59.14s |
| Yükselim: | +26°44'52.4" |
| Görünürdeki Parlaklýk: | 8.015 |
| özdevim Sað Açýklýk: | -15.8 |
| özdevim Yükselim: | -9 |
| B-T magnitude: | 8.459 |
| V-T magnitude: | 8.052 |
Kataloglar ve belirtme:
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