HD51530: found in 3 paper(s).

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/T.V.Mishenina et al.(2002)/ /T.V.Mishenina and V. V. Kovtyukh(2001)/ /J.Simmerer et al.(2004)/

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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

Atmospheric data

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe...-0.39...7.11
Cu I...-0.40+-0.14-0.01+-0.143.81+-0.14
Zn I...-0.26+-0.130.13+-0.134.34+-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 6.20
B-V 0.45

Atmospheric data

Teff 6100
log g 3.8
vturb 0.8

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Mg I...-0.43-0.047.15
Si I...-0.290.107.26
Ca I...-0.240.156.12
Fe...-0.39...7.11
Sr I...-0.40-0.012.57
Ba II...-0.180.211.95
La II...-0.250.140.92
Ce II...-0.340.051.24
Nd II...-0.290.101.21
Eu II...-0.390.000.12
    : 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

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe I...-0.61...6.89
Fe II...-0.7...6.80
La II...-0.460.150.71
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)