G 9-36: found in 3 paper(s).

Labels:

/J.Simmerer et al.(2004)/ /A.M.Boesgaard et al.(2005)/ /A.Stephens and A. M. Boesgaard(2002)/

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A0131

Title The Rise of the s-Process in the Galaxy
ADS J.Simmerer et al.,ApJ, 617, 1091, 2004
Authors J. Simmerer, C. Sneden, J. J. Cowan, J. Collier, V. M. Woolf, J. E. Lawler

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A MCDONALD 60000 100 N/A N/A

Atmospheric data

Teff 5625
log g 4.57
vturb 0.65

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
C...-1.42-0.257.13
Fe I...-1.17...6.33
Fe II...-1.01...6.49
La II...-0.91+-0.110.26+-0.110.26+-0.11
Eu II...-0.67+-0.070.50+-0.07-0.16+-0.07
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

A0193

Title Lithium and Lithium Depletion in Halo Stars on Extreme Orbits
ADS A.M.Boesgaard et al.,ApJ, 633, 398, 2005
Authors A. M. Boesgaard, A. Stephens, C. P. Deliyannis

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A KECKHIRES 48000 140 N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Atmospheric data

Teff 5788+-78
log g 4.35+-0.30
vturb 0.81+-0.13

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li I...0.99+-0.062.03+-0.062.15+-0.06
Fe...-1.04+-0.08...6.46+-0.08
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

A0199

Title ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
ADS A.Stephens et al.,AJ, 123, 1647, 2002
Authors A. Stephens, A. M. Boesgaard

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A 2450820.441 KECKHIRES 48000 140 1000 -48.5+-0.7

Binarity

Vrad -48.5+-0.7

Photometric data

V 11.950
B-V 0.570

Atmospheric data

Teff 5788+-78
log g 4.35+-0.30
vturb 0.81+-0.13

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Na I...-1.17+-0.17-0.06+-0.175.16+-0.17
Mg I...-0.80+-0.05+0.32+-0.076.78+-0.05
Si...-0.94+-0.09+0.18+-0.096.61+-0.09
Si I...-0.93+-0.100.19+-0.106.62+-0.10
Si II...-0.98+-0.160.14+-0.166.57+-0.16
Ca I...-0.89+-0.10+0.23+-0.115.47+-0.10
Ti...-0.90+-0.07+0.22+-0.074.12+-0.07
Ti I...-0.96+-0.070.16+-0.074.06+-0.07
Ti II...-0.80+-0.080.32+-0.084.22+-0.08
Cr...-1.08+-0.07+0.04+-0.074.59+-0.07
Cr I...-1.09+-0.090.03+-0.094.58+-0.09
Cr II...-1.06+-0.090.06+-0.094.61+-0.09
Fe...-1.12+-0.04...6.38+-0.04
Fe I...-1.03+-0.08...6.47+-0.08
Fe II...-1.15+-0.05...6.35+-0.05
Ni I...-1.19+-0.07-0.07+-0.085.06+-0.07
Y II...-1.08+-0.09+0.04+-0.101.16+-0.09
Ba II...-0.95+-0.10+0.17+-0.111.18+-0.10
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)