G 188-30: found in 6 paper(s).
Labels:
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
/M.Ishigaki et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/I.U.Roederer et al.(2014)/
Find this object in SIMBAD
A.M.Boesgaard et al.,ApJ, 633, 398, 2005 (A0193,ADS)
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)
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 |
A.Stephens et al.,AJ, 123, 1647, 2002 (A0199,ADS)
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+-0.1 |
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+-0.1 | 3.35+-0.1 |
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)
Binarity
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 |
Photometric data
M.Ishigaki et al.,PASJ, 62, 143, 2010 (A0229,ADS)
Atmospheric data
Teff : 5326+-39 | log g : 5.00 | vturb : 0.05 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -2.23+-0.06 | -0.59+-0.06 | 4.10+-0.06 |
Mg I | ... | -1.09+-0.20 | 0.55+-0.20 | 6.49+-0.2 |
Ca I | ... | -1.50+-0.03 | 0.14+-0.03 | 4.86+-0.03 |
Ti | ... | -1.37+-0.02 | 0.24+-0.02 | 3.65+-0.02 |
Ti I | ... | -1.44+-0.03 | 0.17+-0.03 | 3.58+-0.03 |
Ti II | ... | -1.24+-0.04 | 0.37+-0.04 | 3.78+-0.04 |
Cr | ... | -1.65+-0.03 | -0.04+-0.03 | 4.02+-0.03 |
Cr I | ... | -1.71+-0.03 | -0.10+-0.03 | 3.96+-0.03 |
Cr II | ... | -1.53+-0.06 | 0.08+-0.06 | 4.14+-0.06 |
Mn I | ... | -2.16+-0.02 | 0.02+-0.02 | 3.23+-0.02 |
Fe I | ... | -1.61+-0.01 | ... | 5.89+-0.01 |
Fe II | ... | -1.75+-0.03 | ... | 5.75+-0.03 |
Ni I | ... | -1.66+-0.07 | -0.03+-0.07 | 4.59+-0.07 |
Zn I | ... | -1.84+-0.07 | -0.21+-0.07 | 2.76+-0.07 |
Y II | ... | -1.74+-0.06 | -0.11+-0.06 | 0.50+-0.06 |
Ba II | ... | -1.78+-0.04 | -0.14+-0.05 | 0.35+-0.04 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-07-27 | N/A | SUBARUHDS | 50000 | 337 | 2400 | -184.2+-0.3 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : +323841.1 | Right Ascension : 215516.15 |
Photometric data
V : 11.03 | V-K : 1.87 | EB-V : 0.02 |
M.N.Ishigaki et al.,ApJ, 753, 64, 2012 (A0273,ADS)
Atmospheric data
Teff : 5379+-100 | log g : 5.00+-0.3 | vturb : 0.09+-0.3 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg | ... | -1.57+-0.13 | 0.06+-0.13 | 6.01+-0.13 |
Ca | ... | -1.53+-0.08 | 0.10+-0.08 | 4.83+-0.08 |
Ti I | ... | -1.36+-0.07 | 0.27+-0.07 | 3.66+-0.07 |
Ti II | ... | -1.24+-0.1 | 0.39+-0.10 | 3.78+-0.1 |
Fe I | ... | -1.63+-0.12 | ... | 5.87+-0.12 |
Fe II | ... | -1.82+-0.12 | ... | 5.68+-0.12 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Binarity
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | SUBARUHDS | 50000 | N/A | N/A | -190.0+-0.3 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : | Right Ascension : |
M.N.Ishigaki et al.,ApJ, 771, 67, 2013 (A0286,ADS)
Atmospheric data
Teff : 5379 | log g : 5 | vturb : 0.09 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Sc II | ... | -1.54+-0.09 | 0.1+-0.09 | 1.63+-0.09 |
Cr I | ... | -1.67+-0.07 | -0.03+-0.07 | 4.00+-0.07 |
Cr II | ... | -1.36+-0.07 | 0.28+-0.07 | 4.31+-0.07 |
Mn I | ... | -1.92+-0.07 | -0.28+-0.07 | 3.47+-0.07 |
Fe I | ... | -1.64+-0.12 | ... | 5.86+-0.12 |
Fe II | ... | -1.82+-0.12 | ... | 5.68+-0.12 |
Ni I | ... | -1.71+-0.11 | -0.07+-0.11 | 4.54+-0.11 |
Cu I | ... | -2.11+-0.12 | -0.47+-0.12 | 2.10+-0.12 |
Zn I | ... | -1.71+-0.17 | -0.07+-0.17 | 2.89+-0.17 |
Y II | ... | -1.61+-0.11 | 0.03+-0.11 | 0.63+-0.11 |
Ba II | ... | -1.61+-0.15 | 0.03+-0.15 | 0.57+-0.15 |
Nd II | ... | -1.05+-0.11 | 0.59+-0.11 | 0.45+-0.11 |
Eu II | ... | -1.46+-0.21 | 0.18+-0.21 | -0.95+-0.21 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 50000 | N/A | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
I.U.Roederer et al.,AJ, 147, 136, 2014 (A0309,ADS)
Atmospheric data
Teff : 5090+-44 | log g : 4.3+-0.2 | vturb : 0.85+-0.13 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <-0.21 | <1.84 | <0.95 |
CH | ... | -2.34+-0.25 | -0.29+-0.25 | 6.07 |
CN | ... | -1.75+-0.28 | 0.3+-0.28 | 6.06 |
Mg I | ... | -1.77+-0.09 | 0.28+-0.09 | 5.83 |
Si I | ... | -1.76+-0.2 | 0.29+-0.2 | 5.75 |
Ca I | ... | -1.79+-0.16 | 0.26+-0.16 | 4.55 |
Sc II | ... | -2.13+-0.12 | -0.08+-0.12 | 1 |
Ti I | ... | -1.89+-0.09 | 0.16+-0.09 | 3.07 |
Ti II | ... | -1.78+-0.1 | 0.27+-0.1 | 3.15 |
V II | ... | -1.99+-0.23 | 0.06+-0.23 | 1.92 |
Cr I | ... | -2.05+-0.1 | 0.00+-0.1 | 3.6 |
Cr II | ... | -1.62+-0.12 | 0.43+-0.12 | 4 |
Mn I | ... | -2.39+-0.1 | -0.34+-0.1 | 3.05 |
Fe I | ... | -2.05+-0.1 | ... | 5.45 |
Fe II | ... | -2.07+-0.11 | ... | 5.43 |
Co I | ... | -2.24+-0.18 | -0.19+-0.18 | 2.76 |
Ni I | ... | -2.08+-0.14 | -0.03+-0.14 | 4.15 |
Zn I | ... | -1.94+-0.1 | 0.11+-0.1 | 2.63 |
Sr II | ... | -2.11+-0.06 | -0.06+-0.06 | 0.74 |
Y II | ... | -2.31+-0.14 | -0.26+-0.14 | -0.12 |
Zr II | ... | -1.71+-0.11 | 0.34+-0.11 | 0.85 |
Mo I | ... | -1.57+-0.18 | 0.48+-0.18 | 0.31 |
Ba II | ... | -2.04+-0.1 | 0.01+-0.1 | 0.12 |
La II | ... | -1.97+-0.19 | 0.08+-0.19 | -0.89 |
Ce II | ... | <-1.57 | <0.48 | <0.01 |
Nd II | ... | -1.76+-0.13 | 0.29+-0.13 | -0.36 |
Sm II | ... | <-1.40 | <0.65 | <-0.39 |
Eu II | ... | <-1.88 | <0.17 | <-1.37 |
Gd II | ... | <-1.08 | <0.97 | <0.04 |
Tb II | ... | <-0.58 | <1.47 | <-0.68 |
Er II | ... | <-1.13 | <0.92 | <-0.2 |
Tm II | ... | <-1.17 | <0.88 | <-1.17 |
Yb II | ... | -1.81+-0.2 | 0.24+-0.2 | -0.91 |
Hf II | ... | <-0.85 | <1.20 | <0.03 |
Pb I | ... | <-1.40 | <0.65 | <0.55 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Binarity
Binarity | Negative |
Vrad | -184.2 |
Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-10-31-02:10 | 2454770.593 | MCDONALD | 33000 | 50-175 | 7200 | -184.7 |
2008-11-02-01:48 | 2454772.577 | MCDONALD | 33000 | 50-175 | 7200 | -183.3 |
2008-11-04-01:26 | 2454774.562 | MCDONALD | 33000 | 50-175 | 5400 | -184.5 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
Photometric data
V : 11.03 | B-V : 0.54 | V-K : 1.63 | EB-V : 0.109 |