HD9430
HIP7217 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 : 5550 | log g : 4.2 | vturb : 0.7 |
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 | ... | -0.01 | ... | -0.40 | 0.06 | 5.84 | Na I |
| Mg I | N/A | ... | 0.32 | ... | -0.18 | 0.28 | 7.42 | Mg I |
| Al I | N/A | ... | 0.25 | ... | -0.21 | 0.25 | 6.24 | Al I |
| Si I | N/A | ... | 0.26 | ... | -0.18 | 0.28 | 7.33 | Si I |
| Ca I | N/A | ... | 0.16 | ... | -0.30 | 0.16 | 6.04 | Ca I |
| Ti | N/A | ... | 0.25 | ... | -0.19 | 0.27 | 4.76 | Ti |
| V I | N/A | ... | 0.1 | ... | -0.31 | 0.15 | 3.62 | V I |
| Cr I | N/A | ... | 0.07 | ... | -0.38 | 0.08 | 5.26 | Cr I |
| Fe | N/A | -0.48 | ... | ... | -0.46 | ... | 7.04 | Fe |
| Ni I | N/A | ... | 0.06 | ... | -0.39 | 0.07 | 5.83 | Ni I |
| Y II | N/A | ... | -0.06 | ... | -0.51 | -0.05 | 1.70 | Y II |
| Zr II | N/A | ... | -0.01 | ... | -0.47 | -0.01 | 2.11 | Zr II |
| Ba II | N/A | ... | -0.07 | ... | -0.60 | -0.14 | 1.58 | Ba II |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 1998-08-08 | 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 : 5725 | log g : 4.36 | vturb : 0.68 |
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 |
|---|
| Mg I | N/A | ... | 0.35+-0.055 | ... | -0.19+-0.055 | 0.19+-0.055 | 7.41+-0.055 | Mg I |
| Si I | N/A | ... | 0.13+-0.048 | ... | -0.22+-0.048 | 0.16+-0.048 | 7.29+-0.048 | Si I |
| Ca I | N/A | ... | 0.15+-0.033 | ... | -0.29+-0.033 | 0.09+-0.033 | 6.05+-0.033 | Ca I |
| Ti I | N/A | ... | 0.24+-0.03 | ... | -0.01+-0.03 | 0.37+-0.03 | 4.94+-0.03 | Ti I |
| Ti II | N/A | ... | 0.15+-0.048 | ... | -0.10+-0.048 | 0.28+-0.048 | 4.85+-0.048 | Ti II |
| Fe I | N/A | -0.37+-0.051 | ... | ... | -0.38+-0.051 | ... | 7.12+-0.051 | Fe I |
| Fe II | N/A | -0.5+-0.066 | ... | ... | -0.51+-0.066 | ... | 6.99+-0.066 | Fe II |
Binary Parameters
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| N/A | N/A | 50000 | >100 | N/A | -53.4 |
| Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : 234144 | Right Ascension : 13258 |
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 | ... | -0.01 | ... | ... | ... | Na |
| Mg | N/A | ... | 0.32 | ... | ... | ... | Mg |
| Ca | N/A | ... | 0.16 | ... | ... | ... | Ca |
| Ti | N/A | ... | 0.25 | ... | ... | ... | Ti |
| Fe | N/A | -0.48 | ... | ... | ... | ... | Fe |
| Ni | N/A | ... | 0.06 | ... | ... | ... | Ni |
| Y | N/A | ... | -0.06 | ... | ... | ... | Y |
| Ba | N/A | ... | -0.07 | ... | ... | ... | Ba |
Observing Log
| Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : +234144 | Right Ascension : 013257.6 |