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A large, complete, volume-limited sample of G-type dwarfs. I. Completion of Stroemgren UVBY photometry
Four-colour photometry of potential dwarf stars of types G0 to K2,selected from the Michigan Spectral Catalogues (Vol. 1-3), has beencarried out. The results are presented in a catalogue containing 4247uvby observations of 3900 stars, all south of δ = -26deg. Theoverall internal rms errors of one observation (transformed to thestandard system) of a program star in the interval 8.5 < V < 10.5are 0.0044, 0.0021, 0.0039, and 0.0059, respectively, in V, b-y, m_1_ ,and c_1_. The purpose of the catalogue, combined with earliercatalogues, is to allow selection of a large, complete, volume-limitedsample of G- and K-type dwarfs, investigate their metallicitydistribution, and compare it to predictions of various models ofgalactic chemical evolution. Future papers in this series will discussthese subjects.
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| Сазвежђа: | Феникс |
| Ректацензија: | 00h05m06.84s |
| Deклинација: | -42°34'04.3" |
| Apparent магнитуда: | 8.974 |
| Даљина: | 195.312 parsecs |
| Proper motion RA: | -65.7 |
| Proper motion Dec: | -23.4 |
| B-T magnitude: | 10.098 |
| V-T magnitude: | 9.067 |
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