BD+13_2698: found in 3 paper(s).

Labels:

/J.P.Fulbright(2000)/ /J.Simmerer et al.(2004)/ /R.Smiljanic et al.(2006)/

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A0126

Title ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
ADS J.P.Fulbright et al.,AJ, 120, 1841, 2000
Authors J. P. Fulbright

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
1998067-8 N/A LICKHAMILTON N/A 70 1200

Photometric data

V 9.37

Atmospheric data

Teff 5500
log g 3.8
vturb 1.05

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Na I...-0.810.165.52
Mg I...-0.480.497.10
Al I...-0.510.465.96
Si I...-0.550.427.00
Ca I...-0.630.345.73
Ti...-0.720.254.30
V I...-0.98-0.013.02
Cr I...-0.920.054.75
Fe...-0.97...6.53
Ni I...-0.890.085.36
Y II...-1.07-0.11.17
Zr II...-0.910.061.69
Ba II...-1.03-0.061.10
Eu II...-0.890.08-0.38
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


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 5705
log g 3.69
vturb 1.30

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe I...-0.90...6.60
Fe II...-0.89...6.61
La II...-0.90+-0.050.00+-0.050.27+-0.05
Eu II...-0.56+-0.040.34+-0.04-0.05+-0.04
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


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 9.37

Atmospheric data

Teff 5500
log g 3.77
vturb 1.05

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li...-0.260.540.9
Be...-0.780.020.37
Fe...-0.8...6.70
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)