HD116316: found in 2 paper(s).
Labels:
/J.P.Fulbright(2000)/
/R.G.Gratton et al.(2003)/
Find this object in SIMBAD

A0126
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 19980317-18 | N/A | LICKHAMILTON | N/A | 230 | 900 | |
Photometric data
Atmospheric data
| Teff | 6250 |
| log g | 4.1 |
| vturb | 1.5 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | 1.10 | 1.77 | 2.26 |
| Na I | ... | -0.53 | 0.14 | 5.80 |
| Mg I | ... | -0.51 | 0.16 | 7.07 |
| Al I | ... | -0.62 | 0.05 | 5.85 |
| Si I | ... | -0.41 | 0.26 | 7.14 |
| Ca I | ... | -0.50 | 0.17 | 5.86 |
| Ti | ... | -0.55 | 0.12 | 4.47 |
| V I | ... | -0.53 | 0.14 | 3.47 |
| Cr I | ... | -0.66 | 0.01 | 5.01 |
| Fe | ... | -0.67 | ... | 6.83 |
| Ni I | ... | -0.65 | 0.02 | 5.60 |
| Y II | ... | -0.70 | -0.03 | 1.54 |
| Zr II | ... | -0.65 | 0.02 | 1.95 |
| Ba II | ... | -0.42 | 0.25 | 1.71 |
| Eu II | ... | -0.40 | 0.27 | 0.11 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0135
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | N/A | N/A | N/A | N/A | N/A | -28 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | 260657 |
| Right Ascension | 132234 |
Photometric data
Atmospheric data
| Teff | 6258 |
| log g | 4.19 |
| vturb | 1.4 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| Na I | ... | -0.52+-0.054 | 0.19+-0.054 | 5.81+-0.054 |
| Mg I | ... | -0.46+-0.055 | 0.25+-0.055 | 7.12+-0.055 |
| Si I | ... | -0.48+-0.048 | 0.23+-0.048 | 7.07+-0.048 |
| Ca I | ... | -0.49+-0.033 | 0.22+-0.033 | 5.87+-0.033 |
| Ti I | ... | -0.69+-0.03 | 0.02+-0.03 | 4.33+-0.03 |
| Ti II | ... | -0.62+-0.048 | 0.09+-0.048 | 4.40+-0.048 |
| Fe I | ... | -0.71+-0.051 | ... | 6.79+-0.051 |
| Fe II | ... | -0.66+-0.066 | ... | 6.84+-0.066 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)