HE0926-0508: found in 2 paper(s).
Labels:
/P.S.Barklem et al.(2005)/
/A.Frebel et al.(2006)/
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A0052
| Title | The Hamburg/ESO R-process enhanced star survey (HERES). II. Spectroscopic analysis of the survey sample |
| ADS | P.S.Barklem et al.,AAP, 439, 129, 2005 |
| Authors | P. S. Barklem, N. Christlieb, T. C. Beers, V. Hill, M. S. Bessell, J. Holmberg, B. Marsteller, S. Rossi, F. -J. Zickgraf, D. Reimers |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | N/A | VLT | 20000 | 124 | N/A | 191.0 |
Atmospheric data
| Teff | 6249 |
| log g | 4.24 |
| vturb | 1.60 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -2.32+-0.23 | 0.62+-0.27 | 6.23+-0.23 |
| Mg | ... | -2.50+-0.23 | 0.28+-0.23 | 5.08+-0.18 |
| Al | ... | -3.68+-0.20 | -0.90+-0.24 | 2.79+-0.20 |
| Ca | ... | -2.40+-0.19 | 0.37+-0.24 | 3.96+-0.19 |
| Sc | ... | -2.50+-0.25 | 0.28+-0.25 | 0.67+-0.22 |
| Ti | ... | -2.29+-0.24 | 0.49+-0.24 | 2.73+-0.21 |
| Cr | ... | -2.92+-0.19 | -0.14+-0.22 | 2.75+-0.19 |
| Mn | ... | -3.32+-0.23 | -0.54+-0.23 | 2.07+-0.19 |
| Fe | ... | -2.78+-0.17 | 0.00+-0.22 | 4.72+-0.17 |
| Ni | ... | -2.84+-0.22 | -0.06+-0.22 | 3.42+-0.19 |
| Sr | ... | -2.80+-0.27 | -0.02+-0.27 | 0.17+-0.26 |
| Ba | ... | -3.05+-0.22 | -0.28+-0.25 | -0.92+-0.22 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0095
| Title | Bright Metal-poor Stars from the Hamburg/ESO Survey. I. Selection and Follow-up Observations from 329 Fields |
| ADS | A.Frebel et al.,ApJ, 652, 1585, 2006 |
| Authors | A. Frebel, N. Christlieb, J. E. Norris, T. C. Beers, M. S. Bessell, J. Rhee, C. Fechner, B. Marsteller, S. Rossi, C. Thom, L. Wisotzki, D. Reimers |
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Basic Informations
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -052139 |
| Right Ascension | 092855.2 |
Photometric data
| B | 12.7 |
| B-V | 0.47 |
| EB-V | 0.04 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| Fe | ... | -2.80 | ... | 4.70 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)