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Narrow-band photometry of G and K stars near the North Galactic Pole
Photoelectric narrow-band photometry obtained for 292 late-type starsbrighter than 10 m in the North Galactic Pole area is discussed. The g,n, k, m, f-system of Dickow et al. (1970) is used. The stars were chosenfrom two lists: (1) all stars of spectral type G5 or later in the HenryDraper Catalog (Cannon and Pickering, 1918-1924) within 15 deg of theNorth Galactic Pole, together with a few BD stars; and (2) all starsclassified as K or M giants and in Upgren's 25-31 deg zones (Upgren,1962). For most of the stars, estimates of the following quantities arederived: V-magnitude, R-I color, metal abundance, MV, and theduplicity parameter res(k).
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Berenisin Saci |
| Sað Açýklýk: | 13h21m35.15s |
| Yükselim: | +18°13'29.4" |
| Görünürdeki Parlaklýk: | 8.714 |
| Uzaklýk: | 606.061 parsek |
| özdevim Sað Açýklýk: | -11.4 |
| özdevim Yükselim: | -8 |
| B-T magnitude: | 10.178 |
| V-T magnitude: | 8.835 |
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