G 188-30: found in 2 paper(s).
Labels:
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
Find this object in SIMBAD

A0193
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 48000 | 350 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 5141+-40 |
log g | 4.44+-0.25 |
vturb | 0.31+-0.34 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | -0.34+-0.04 | 1.55+-0.04 | 0.82+-0.04 |
Fe | ... | -1.89+-0.06 | ... | 5.61+-0.06 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0199
Get more information of this paper.
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | 2449904.618 | KECKHIRES | 48000 | 350 | 900 | -185.0+-0.7 |
N/A | 2450289.483 | KECKHIRES | 48000 | 350 | 2100 | -184.8+-0.7 |
Binarity
Photometric data
Atmospheric data
Teff | 5141+-40 |
log g | 4.44+-0.25 |
vturb | 0.31+-0.34 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -2.12+-0.18 | -0.23+-0.19 | 4.21+-0.18 |
Mg I | ... | -1.56+-0.08 | +0.34+-0.09 | 6.02+-0.08 |
Si | ... | -1.71+-0.18 | +0.19+-0.18 | 5.84+-0.18 |
Si I | ... | -1.71+-0.17 | 0.19+-0.17 | 5.84+-0.17 |
Ca I | ... | -1.70+-0.10 | +0.20+-0.11 | 4.66+-0.10 |
Ti | ... | -1.72+-0.08 | +0.18+-0.08 | 3.30+-0.08 |
Ti I | ... | -1.75+-0.08 | 0.15+-0.08 | 3.27+-0.08 |
Ti II | ... | -1.67+-0.10 | 0.23+-0.10 | 3.35+-0.10 |
Cr | ... | -1.88+-0.07 | +0.02+-0.07 | 3.79+-0.07 |
Cr I | ... | -1.89+-0.05 | 0.01+-0.05 | 3.78+-0.05 |
Cr II | ... | -1.79+-0.13 | 0.11+-0.13 | 3.88+-0.13 |
Fe | ... | -1.90+-0.05 | ... | 5.60+-0.05 |
Fe I | ... | -1.87+-0.07 | ... | 5.63+-0.07 |
Fe II | ... | -1.95+-0.09 | ... | 5.55+-0.09 |
Ni I | ... | -1.99+-0.09 | -0.09+-0.10 | 4.26+-0.09 |
Y II | ... | -2.05+-0.06 | -0.15+-0.08 | 0.19+-0.06 |
Ba II | ... | -1.97+-0.05 | -0.07+-0.08 | 0.16+-0.05 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)