HD203608: found in 3 paper(s).

Labels:

/K.Jonsell et al.(2005)/ /M.Takada-Hidai et al.(2002)/ /R.Smiljanic et al.(2006)/

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A0078

Title Chemical abundances in 43 metal-poor stars
ADS K.Jonsell et al.,AAP, 440, 321, 2005
Authors K. Jonsell, B. Edvardsson, B. Gustafsson, P. Magain, P. E. Nissen, M. Asplund

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A CATCESESO 60000 200 N/A N/A
Galactic Longitude (l) 328.157
Galactic Latitude (b) -40.292
Declination -65.3662
Right Ascension 321.6109

Photometric data

V 4.229

Atmospheric data

Teff 6063
log g 4.29
vturb 1.5

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
O I...-0.420.328.45
Na I...-0.570.175.76
Mg I...-0.570.177.01
Al I...-0.630.115.84
Si I...-0.630.116.92
Ca I...-0.640.105.72
Sc II...-0.700.042.47
V I...-0.610.133.39
Cr I...-0.740.004.93
Fe...-0.74...6.76
Fe II......-0.01...
Ni I...-0.730.015.52
Ba II...-0.85-0.111.28
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0184

Title Behavior of Sulfur Abundances in Metal-poor Giants and Dwarfs
ADS M.Takada-Hidai et al.,ApJ, 573, 614, 2002
Authors M. Takada-Hidai, Y. Takeda, S. Sato, S. Honda, K. Sadakane, S. Kawanomoto, W. L.W. Sargent, L. Lu, T. A. Barlow

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Photometric data

V 4.21
EB-V 0.00

Atmospheric data

Teff 6070+-100
log g 4.27+-0.15
vturb 1.6+-0.5

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
S I...-0.710.346.50
Fe I...-1.05...6.46
    : 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 4.22

Atmospheric data

Teff 6139
log g 4.26
vturb 1.57

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li...1.231.902.39
Be...-0.470.200.68
Fe...-0.67...6.83
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)