BPS CS30312-059: found in 2 paper(s).
Labels:
/W.Aoki et al.(2005)/
/D.K.Lai et al.(2008)/
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A0057
| Title | Spectroscopic Studies of Very Metal-poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements |
| ADS | W.Aoki et al.,ApJ, 632, 611, 2005 |
| Authors | W. Aoki, S. Honda, T. C. Beers, T. Kajino, H. Ando, J. E. Norris, S. G. Ryan, H. Izumiura, K. Sadakane, M. Takada-Hidai |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2001-07-23 | N/A | SUBARUHDS | 50000 | 144 | 60min | -155.94+-0.21 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | -012338 |
| Right Ascension | 153448.8 |
Binarity
Photometric data
| V | 13.101 |
| B | 13.904 |
| H | 10.826 |
| J | 11.305 |
| K | 10.723 |
| EB-V | 0.08 |
Atmospheric data
| Teff | 4950 |
| log g | 2.0 |
| vturb | 1.8 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -2.74 | 0.3 | 5.6 |
| Mg I | ... | -2.48+-0.1 | 0.56+-0.1 | 5.1+-0.1 |
| Al I | ... | -3.85+-0.17 | -0.81+-0.17 | 2.64+-0.17 |
| Si I | ... | -2.45+-0.12 | 0.59+-0.12 | 5.11+-0.12 |
| Ca I | ... | -2.69+-0.1 | 0.35+-0.1 | 3.66+-0.1 |
| Sc II | ... | -2.93+-0.22 | 0.11+-0.22 | 0.17+-0.22 |
| Ti I | ... | -2.78+-0.1 | 0.26+-0.1 | 2.16+-0.1 |
| Ti II | ... | -2.62+-0.24 | 0.42+-0.24 | 2.32+-0.24 |
| Cr I | ... | -3.48+-0.08 | -0.44+-0.08 | 2.21+-0.08 |
| Mn I | ... | -3.98+-0.18 | -0.94+-0.18 | 1.55+-0.18 |
| Fe I | ... | -3.04+-0.2 | ... | 4.46+-0.2 |
| Fe II | ... | -3.02+-0.19 | ... | 4.48+-0.19 |
| Co I | ... | -2.72+-0.1 | 0.32+-0.1 | 2.19+-0.1 |
| Ni I | ... | -3.12+-0.09 | -0.08+-0.09 | 3.13+-0.09 |
| Zn I | ... | -2.73+-0.2 | 0.31+-0.2 | 1.94+-0.2 |
| Sr II | ... | -2.85+-0.23 | 0.19+-0.23 | 0.07+-0.23 |
| Y II | ... | -3.02+-0.23 | 0.02+-0.23 | -0.79+-0.23 |
| Zr II | ... | -2.76+-0.25 | 0.28+-0.25 | -0.15+-0.25 |
| Ba II | ... | -3.35+-0.2 | -0.31+-0.2 | -1.13+-0.2 |
| Nd II | ... | -2.94+-0.24 | 0.1+-0.24 | -1.45+-0.24 |
| Eu II | ... | -2.50+-0.24 | 0.54+-0.24 | -1.95+-0.24 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0181
| Title | Detailed Abundances for 28 Metal-poor Stars: Stellar Relics in the Milky Way |
| ADS | D.K.Lai et al.,ApJ, 681, 1524, 2008 |
| Authors | D. K. Lai, M. Bolte, J. A. Johnson, S. Lucatello |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2004-04-08 | N/A | KECKHIRES | N/A | 134 | 3600 | -156.4+-0.2 |
| 2004-04-09 | N/A | KECKHIRES | N/A | 169 | 4800 | -155.2+-0.2 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 5021+-100 |
| log g | 2.06+-0.2 |
| vturb | 1.8+-0.2 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -2.87+-0.13 | 0.27+-0.13 | 5.68+-0.13 |
| N | ... | <-3.62 | <-0.48 | <4.35 |
| Na | ... | -2.97+-0.08 | 0.17+-0.08 | 3.36+-0.08 |
| Mg | ... | -2.73+-0.06 | 0.41+-0.06 | 4.85+-0.06 |
| Al | ... | -4.02+-0.06 | -0.88+-0.06 | 2.45+-0.06 |
| Ca | ... | -2.81+-0.05 | 0.33+-0.05 | 3.55+-0.05 |
| Sc II | ... | -3.07+-0.06 | 0.07+-0.06 | 0.10+-0.06 |
| Ti I | ... | -2.83+-0.07 | 0.31+-0.07 | 2.19+-0.07 |
| Ti II | ... | -2.75+-0.06 | 0.39+-0.06 | 2.27+-0.06 |
| V II | ... | -3.10+-0.07 | 0.04+-0.07 | 0.90+-0.07 |
| Cr I | ... | -3.48+-0.09 | -0.34+-0.09 | 2.19+-0.09 |
| Cr II | ... | -3.05+-0.16 | 0.09+-0.16 | 2.62+-0.16 |
| Mn I | ... | -4.02+-0.10 | -0.88+-0.10 | 1.37+-0.10 |
| Mn II | ... | -3.67+-0.06 | -0.53+-0.06 | 1.72+-0.06 |
| Fe I | ... | -3.14+-0.09 | ... | 4.36+-0.09 |
| Fe II | ... | -3.19+-0.08 | ... | 4.31+-0.08 |
| Co | ... | -2.86+-0.07 | 0.28+-0.07 | 2.06+-0.07 |
| Ni | ... | -3.19+-0.06 | -0.05+-0.06 | 3.06+-0.06 |
| Sr II | ... | -3.16+-0.17 | -0.02+-0.17 | -0.19+-0.17 |
| Y II | ... | -3.15+-0.08 | -0.01+-0.08 | -0.91+-0.08 |
| Zr II | ... | -2.79+-0.08 | 0.35+-0.08 | -0.19+-0.08 |
| Ba II | ... | -3.15+-0.08 | -0.01+-0.08 | -1.02+-0.08 |
| Eu II | ... | -2.51+-0.11 | 0.63+-0.11 | -2.00+-0.11 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)