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Bright Metal-poor Stars from the Hamburg/ESO Survey. I. Selection and Follow-up Observations from 329 Fields
We present a sample of 1777 bright (91.0) metal-poor([Fe/H]<-2.0) giants of 9%+/-2%, which is lower than previouslyreported. However, the frequency rises to similar (>20%) and highervalues with increasing distance from the Galactic plane. Although thenumbers of stars at low metallicity are falling rapidly at the lowestmetallicities, there is evidence that the fraction of carbon-enhancedmetal-poor stars is increasing rapidly as a function of decliningmetallicity. For ~60 objects, high-resolution data have already beenobtained; one of these, HE 1327-2326, is the new record holder for themost iron-deficient star known.
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Miembro de los siguientes grupos:
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Datos observacionales y astrométricos
| Constelación: | Cincel |
| Ascensión Recta: | 04h36m55.19s |
| Declinación: | -41°15'41.4" |
| Magnitud Aparente: | 9.944 |
| Movimiento Propio en Ascensión Recta: | 2.5 |
| Movimiento Propio en Declinación: | 22 |
| B-T magnitude: | 10.469 |
| V-T magnitude: | 9.988 |
Catálogos y designaciones:
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INHABITED SKY
