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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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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Coma Berenices |
| Ascensió Recta: | 12h54m05.29s |
| Declinació: | +15°19'47.5" |
| Magnitud Aparent: | 8.719 |
| Distancia: | 342.466 parsecs |
| Moviment propi RA: | -8 |
| Moviment propi Dec: | -28.5 |
| B-T magnitude: | 10.216 |
| V-T magnitude: | 8.843 |
Catàlegs i designacions:
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