HD018768: found in 3 paper(s).

Labels:

/T.V.Mishenina et al.(2002)/ /T.V.Mishenina et al.(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...-0.51...6.99
Cu I...-0.63+-0.25-0.12+-0.253.58+-0.25
Zn I...-0.30+-0.230.21+-0.234.30+-0.23
    : 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 6.72
B-V 0.59

Atmospheric data

Teff 5700
log g 3.5
vturb 1.0

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Mg I...-0.510.007.07
Si I...-0.410.107.14
Ca I...-0.360.156.00
Fe...-0.51...6.99
Sr I...-0.55-0.042.42
Ba II...-0.290.221.84
La II...-0.480.030.69
Ce II...-0.57-0.061.01
Nd II...-0.500.011.00
Eu II...-0.250.260.26
    : 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...-0.65...6.85
Fe II...-0.71...6.79
La II...-0.72-0.070.45
Eu II...-0.580.07-0.07
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)