HE1300+0157: found in 2 paper(s).
Labels:
/P.S.Barklem et al.(2005)/
/A.Frebel et al.(2007)/
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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 | 56 | N/A | 73.6 |
Atmospheric data
| Teff | 5411 |
| log g | 3.38 |
| vturb | 1.43 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -2.73+-0.27 | 1.17+-0.29 | 5.82+-0.27 |
| Mg | ... | -3.34+-0.27 | 0.40+-0.27 | 4.25+-0.24 |
| Al | ... | -4.57+-0.22 | -0.83+-0.27 | 1.90+-0.22 |
| Ca | ... | -3.26+-0.22 | 0.47+-0.25 | 3.10+-0.22 |
| Sc | ... | -3.48+-0.29 | 0.26+-0.29 | -0.30+-0.24 |
| Ti | ... | -3.40+-0.28 | 0.34+-0.28 | 1.62+-0.22 |
| Cr | ... | -4.11+-0.20 | -0.37+-0.25 | 1.56+-0.20 |
| Fe | ... | -3.74+-0.19 | 0.00+-0.22 | 3.76+-0.19 |
| Co | ... | -3.23+-0.25 | 0.50+-0.30 | 1.69+-0.25 |
| Ni | ... | -3.78+-0.23 | -0.04+-0.23 | 2.48+-0.17 |
| Y | ... | -3.18+-0.31 | 0.56+-0.31 | -0.94+-0.22 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0112
| Title | Chemical Abundance Analysis of the Extremely Metal-poor Star HE 1300+0157 |
| ADS | A.Frebel et al.,ApJ, 658, 534, 2007 |
| Authors | A. Frebel, J. E. Norris, W. Aoki, S. Honda, M. S. Bessell, M. Takada-Hidai, T. C. Beers, N. Christlieb |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2004-05-30-0737 | N/A | SUBARUHDS | 60000 | 70-170 | 30min | 75.3 |
| 2004-06-01-0539 | N/A | SUBARUHDS | 60000 | 70-170 | 270min | 74.6 |
| 2005-03-02-1208 | N/A | SUBARUHDS | 60000 | 35-70 | 180min | 74.6 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
| V | 14.060+-0.004 |
| B-V | 0.476+-0.009 |
| V-R | 0.799+-0.006 |
| J-H | 0.390+-0.036 |
| J-K | 0.458+-0.040 |
| V-K | 1.709+-0.029 |
| R-I | 0.417+-0.009 |
| EB-V | 0.022 |
Atmospheric data
| Teff | 5450+-70 |
| log g | 3.2+-0.3 |
| vturb | 1.54+-0.3 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Li I | ... | -0.10+-0.09 | 3.63+-0.09 | 1.06+-0.09 |
| CH | ... | -2.50+-0.27 | 1.38+-0.27 | 5.89+-0.27 |
| NH | ... | <-2.66 | <1.22 | <5.12 |
| OH | ... | -2.12+-0.39 | 1.76+-0.39 | 6.54+-0.39 |
| Na I | ... | -3.73+-0.10 | 0.15+-0.10 | 2.44+-0.10 |
| Mg I | ... | -3.43+-0.14 | 0.45+-0.14 | 4.10+-0.14 |
| Al I | ... | -4.33+-0.12 | -0.45+-0.12 | 2.04+-0.12 |
| Si I | ... | -3.01+-0.18 | 0.87+-0.18 | 4.50+-0.18 |
| Ca I | ... | -3.33+-0.12 | 0.55+-0.12 | 2.98+-0.12 |
| Ca II | ... | -3.56+-0.14 | 0.32+-0.14 | 2.75+-0.14 |
| Sc II | ... | -3.42+-0.15 | 0.46+-0.15 | -0.37+-0.15 |
| Ti I | ... | -3.24+-0.14 | 0.64+-0.14 | 1.66+-0.14 |
| Ti II | ... | -3.13+-0.16 | 0.75+-0.16 | 1.77+-0.16 |
| V I | ... | <-2.85 | <1.03 | <1.15 |
| Cr I | ... | -4.13+-0.15 | -0.25+-0.15 | 1.51+-0.15 |
| Cr II | ... | -3.99+-0.13 | -0.11+-0.13 | 1.65+-0.13 |
| Mn I | ... | -4.34+-0.13 | -0.46+-0.13 | 1.05+-0.13 |
| Mn II | ... | -4.50+-0.13 | -0.62+-0.13 | 0.89+-0.13 |
| Fe I | ... | -3.73+-0.16 | 0.15+-0.16 | 3.72+-0.16 |
| Fe II | ... | -3.88+-0.14 | 0.00+-0.14 | 3.57+-0.14 |
| Co I | ... | -3.12+-0.15 | 0.76+-0.15 | 1.80+-0.15 |
| Ni I | ... | -3.62+-0.20 | 0.26+-0.20 | 2.61+-0.20 |
| Zn I | ... | <-2.97 | <0.91 | <1.63 |
| Sr II | ... | <-5.56 | <-1.68 | <-2.64 |
| Y II | ... | <-3.14 | <0.74 | <-0.93 |
| Zr II | ... | <-2.66 | <1.22 | <-0.07 |
| Ba II | ... | <-4.73 | <-0.85 | <-2.56 |
| Eu II | ... | <-2.32 | <1.56 | <-1.80 |
| Pb I | ... | <-1.10 | <2.78 | <0.90 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)