G 170-21: found in 3 paper(s).

Labels:

/R.Smiljanic et al.(2006)/ /A.M.Boesgaard et al.(2005)/ /A.Stephens and A. M. Boesgaard(2002)/

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A0190

Title Beryllium abundances and star formation in the halo and in the thick disk
ADS R.Smiljanic et al.,ApJ, 644, L121, 2006
Authors R. Smiljanic, L. Pasquini, P. Bonifacio, D. Galli, R. G. Gratton, S. Randich, B. Wolff

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Photometric data

V 12.51

Atmospheric data

Teff 5664
log g 4.65
vturb 0.00

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li...0.752.201.91
Be...-0.730.720.42
Fe...-1.45...6.05
    : 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 100 N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Atmospheric data

Teff 5664+-95
log g 4.65+-0.29
vturb 0.00+-0.50

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li I...0.72+-0.072.17+-0.071.88+-0.07
Fe...-1.45+-0.10...6.05+-0.10
    : 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 2450240.486 KECKHIRES 48000 100 1800 -222.0+-0.9

Binarity

Vrad -222.0+-0.9

Photometric data

V 12.580
B-V 0.600

Atmospheric data

Teff 5664+-95
log g 4.65+-0.29
vturb 0.00+-0.50

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Na I...-1.53+-0.14-0.06+-0.164.80+-0.14
Mg I...-0.98+-0.16+0.49+-0.176.60+-0.16
Si...-1.26+-0.09+0.21+-0.096.29+-0.09
Si I...-1.28+-0.070.19+-0.076.27+-0.07
Si II...-1.08+-0.160.39+-0.166.47+-0.16
Ca I...-1.16+-0.13+0.31+-0.155.20+-0.13
Ti...-1.18+-0.10+0.29+-0.103.84+-0.10
Ti I...-1.20+-0.100.27+-0.103.82+-0.10
Ti II...-1.16+-0.090.31+-0.093.86+-0.09
Cr...-1.45+-0.10+0.02+-0.104.22+-0.10
Cr I...-1.48+-0.09-0.01+-0.094.19+-0.09
Cr II...-1.31+-0.190.16+-0.194.36+-0.19
Fe...-1.47+-0.07...6.03+-0.07
Fe I...-1.44+-0.08...6.06+-0.08
Fe II...-1.52+-0.12...5.98+-0.12
Ni I...-1.55+-0.13-0.09+-0.144.70+-0.13
Y II...-1.32+-0.09+0.15+-0.110.92+-0.09
Ba II...-1.28+-0.09+0.19+-0.110.85+-0.09
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)