HD157089: found in 3 paper(s).

Labels:

/T.V.Mishenina et al.(2002)/ /T.V.Mishenina and V. V. Kovtyukh(2001)/ /M.Takada-Hidai et al.(2002)/

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A0070

Title Abundances of Cu and Zn in metal-poor stars: Clues for Galaxy evolution
ADS T.V.Mishenina et al.,AAP, 396, 189, 2002
Authors T. V. Mishenina, V. V. Kovtyukh, C. Soubiran, C. Travaglio, M. Busso

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A ELODIE 42000 >100 N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe...-0.58...6.92
Cu I...-0.60+-0.14-0.02+-0.143.61+-0.14
Zn I...-0.50+-0.130.08+-0.134.10+-0.13
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0071

Title Analysis of neutron capture elements in metal-poor stars
ADS T.V.Mishenina et al.,AAP, 370, 951, 2001
Authors T. V. Mishenina, V. V. Kovtyukh

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A ELODIE 42000 >100 N/A N/A

Photometric data

V 6.95
B-V 0.60

Atmospheric data

Teff 5785
log g 3.8
vturb 1.0

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Mg I...-0.450.117.13
Si I...-0.360.207.19
Ca I...-0.340.226.02
Fe...-0.56...6.94
Sr I...-0.57-0.012.40
Ba II...-0.550.011.58
La II...-0.62-0.060.55
Ce II...-0.520.041.06
Nd II...-0.480.081.02
    : 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 6.95
EB-V 0.02

Atmospheric data

Teff 5840+-100
log g 4.01+-0.15
vturb 1.8+-0.5

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
S I...-0.480.466.73
Fe I...-0.94...6.57
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)