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Detailed analysis of cool stars
An analysis of 14 cool stars is presented, nine of which have beenpreviously found to be associated with moving groups and five which arecharacterized by large spatial velocity. The results suggest that themoving groups Zeta Her, Wolf 630, and Kapteyn could really exist.Although no peculiar abundance relative to iron is found, a relativeoverabundance of Ni is noted for the most metal poor stars in thesample.
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Membre dels grups següents:
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Dades d'Observació i Astrometria
| Constel·lació: | Capricornus |
| Ascensió Recta: | 21h22m24.11s |
| Declinació: | -25°09'51.0" |
| Magnitud Aparent: | 9.289 |
| Moviment propi RA: | 39.6 |
| Moviment propi Dec: | -25.9 |
| B-T magnitude: | 9.659 |
| V-T magnitude: | 9.32 |
Catàlegs i designacions:
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INHABITED SKY
