HD129392
HIP71886 in K.A.Venn+,AJ, 128, 1177, 2004
taken from 3 paper(s):
/J.P.Fulbright(2000)/
/R.G.Gratton et al.(2003)/
/K.A.Venn et al.(2004)/
J.P.Fulbright et al.,AJ, 120, 1841, 2000 (A0126,ADS)
ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
Stellar Parameters
| Teff : 6400 | log g : 4.1 | vturb : 1.5 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
|---|
| Li I | N/A | ... | ... | 2.07 | -1.19 | -0.81 | 2.07 | Li I |
| Na I | N/A | ... | 0.1 | ... | -0.21 | 0.17 | 6.03 | Na I |
| Mg I | N/A | ... | 0.12 | ... | -0.30 | 0.08 | 7.30 | Mg I |
| Al I | N/A | ... | -0.01 | ... | -0.39 | -0.01 | 6.06 | Al I |
| Si I | N/A | ... | 0.19 | ... | -0.17 | 0.21 | 7.34 | Si I |
| Ca I | N/A | ... | 0.08 | ... | -0.30 | 0.08 | 6.04 | Ca I |
| Ti | N/A | ... | 0.04 | ... | -0.32 | 0.06 | 4.63 | Ti |
| V I | N/A | ... | 0.13 | ... | -0.20 | 0.18 | 3.73 | V I |
| Cr I | N/A | ... | 0.03 | ... | -0.34 | 0.04 | 5.30 | Cr I |
| Fe | N/A | -0.4 | ... | ... | -0.38 | ... | 7.12 | Fe |
| Y II | N/A | ... | -0.07 | ... | -0.44 | -0.06 | 1.77 | Y II |
| Zr II | N/A | ... | 0.06 | ... | -0.32 | 0.06 | 2.26 | Zr II |
| Ba II | N/A | ... | 0.29 | ... | -0.16 | 0.22 | 2.02 | Ba II |
| Eu II | N/A | ... | 0.28 | ... | -0.13 | 0.25 | 0.39 | Eu II |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 19980317-18 | N/A | LICKHAMILTON | 50000 | 115 | 1500 | N/A |
| Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
R.G.Gratton et al.,AAP, 404, 187, 2003 (A0135,ADS)
Abundances for metal-poor stars with accurate parallaxes
Stellar Parameters
| Teff : 6698 | log g : 4.4 | vturb : 1.35 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
|---|
| Na I | N/A | ... | 0.03+-0.054 | ... | -0.22+-0.054 | 0.01+-0.054 | 6.02+-0.054 | Na I |
| Mg I | N/A | ... | 0.12+-0.055 | ... | -0.27+-0.055 | -0.04+-0.055 | 7.33+-0.055 | Mg I |
| Si I | N/A | ... | 0.04+-0.048 | ... | -0.16+-0.048 | 0.07+-0.048 | 7.35+-0.048 | Si I |
| Ca I | N/A | ... | 0.06+-0.033 | ... | -0.23+-0.033 | -0.00+-0.033 | 6.11+-0.033 | Ca I |
| Ti I | N/A | ... | -0.04+-0.03 | ... | -0.14+-0.03 | 0.09+-0.03 | 4.81+-0.03 | Ti I |
| Fe I | N/A | -0.22+-0.051 | ... | ... | -0.23+-0.051 | ... | 7.27+-0.051 | Fe I |
| Fe II | N/A | -0.31+-0.066 | ... | ... | -0.32+-0.066 | ... | 7.18+-0.066 | Fe II |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| N/A | N/A | 50000 | >100 | N/A | -16 |
| Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : 35619 | Right Ascension : 144211 |
K.A.Venn et al.,AJ, 128, 1177, 2004 (C0011,ADS)
Stellar Chemical Signatures and Hierarchical Galaxy Formation
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
|---|
| Na | N/A | ... | 0.1 | ... | ... | ... | Na |
| Mg | N/A | ... | 0.12 | ... | ... | ... | Mg |
| Ca | N/A | ... | 0.08 | ... | ... | ... | Ca |
| Ti | N/A | ... | 0.04 | ... | ... | ... | Ti |
| Fe | N/A | -0.4 | ... | ... | ... | ... | Fe |
| Y | N/A | ... | -0.07 | ... | ... | ... | Y |
| Ba | N/A | ... | 0.29 | ... | ... | ... | Ba |
| Eu | N/A | ... | 0.28 | ... | ... | ... | Eu |
Observing Log
| Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : +035619 | Right Ascension : 144211.2 |