HE1120-0153: 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 | 194 | N/A | 228.4 |
Atmospheric data
| Teff | 6191 |
| log g | 4.09 |
| vturb | 0.68 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -2.29+-0.23 | 0.63+-0.26 | 6.26+-0.23 |
| Mg | ... | -2.72+-0.23 | 0.04+-0.23 | 4.86+-0.17 |
| Al | ... | -3.83+-0.20 | -1.07+-0.25 | 2.64+-0.20 |
| Ca | ... | -2.56+-0.19 | 0.20+-0.24 | 3.80+-0.19 |
| Sc | ... | -2.56+-0.25 | 0.20+-0.25 | 0.61+-0.22 |
| Ti | ... | -2.46+-0.25 | 0.30+-0.25 | 2.56+-0.21 |
| Cr | ... | -2.98+-0.19 | -0.22+-0.22 | 2.69+-0.19 |
| Mn | ... | -3.45+-0.23 | -0.69+-0.23 | 1.94+-0.19 |
| Fe | ... | -2.76+-0.17 | 0.00+-0.22 | 4.74+-0.17 |
| Ni | ... | -2.95+-0.22 | -0.19+-0.22 | 3.30+-0.19 |
| Sr | ... | -2.94+-0.27 | -0.18+-0.27 | 0.03+-0.25 |
| Ba | ... | -2.89+-0.20 | -0.13+-0.24 | -0.76+-0.20 |
: 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 | -020936 |
| Right Ascension | 112243.2 |
Photometric data
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| Fe | ... | -2.79 | ... | 4.71 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)