HD345957: found in 5 paper(s).

Labels:

/R.G.Gratton et al.(2000)/ /T.V.Mishenina et al.(2002)/ /T.V.Mishenina et al.(2001)/ /J.P.Fulbright(2000)/ /R.G.Gratton et al.(2003)/

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A0049

Title Mixing along the red giant branch in metal-poor field stars
ADS R.G.Gratton et al.,AAP, 354, 169, 2000
Authors R. G. Gratton, C. Sneden, E. Carretta, A. Bragaglia

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
1995-05 N/A CESESO 50000 80-150 N/A N/A
1995-11 N/A CESESO 50000 80-150 N/A N/A
1995-11 N/A MCDONALD 60000 70-100 N/A N/A
Galactic Longitude (l) 063.26
Galactic Latitude (b) -05.21
Declination +235755
Right Ascension 201048.2

Photometric data

V 8.88
B-V 0.510

Atmospheric data

Teff 5845
log g 3.91
vturb 1.20

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe I...-1.39...6.11
Fe II...-1.37...6.13
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

Isotope ratio

12C/13C >20

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...-1.33...6.17
Cu I...-1.60+-0.13-0.27+-0.132.61+-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 8.89
B-V 0.51

Atmospheric data

Teff 5800
log g 3.7
vturb 1.0

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Mg I...-1.250.086.33
Si I...-1.120.216.43
Ca I...-1.000.335.36
Fe...-1.33...6.17
Sr I...-1.080.251.89
Ba II...-0.970.361.16
Ce II...-0.980.350.60
Nd II...-0.990.340.51
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

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
1998-08-08 N/A LICKHAMILTON N/A 110 1200

Photometric data

V 8.9

Atmospheric data

Teff 5650
log g 3.8
vturb 1.3

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li I...1.272.772.43
Na I...-1.65-0.154.68
Mg I...-1.090.416.49
Si I...-1.040.466.51
Ca I...-1.120.385.24
Ti...-1.160.343.86
V I...-1.57-0.072.43
Cr I...-1.55-0.054.12
Fe...-1.5...6.00
Ni I...-1.51-0.014.74
Y II...-1.480.020.76
Zr II...-1.160.341.44
Ba II...-1.420.080.71
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

A0135

Title Abundances for metal-poor stars with accurate parallaxes
ADS R.G.Gratton et al.,AAP, 404, 187, 2003
Authors R. G. Gratton, E. Carretta, R. Claudi, S. Lucatello, M. Barbieri

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A N/A N/A N/A N/A -110.5
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination 235755
Right Ascension 201048

Photometric data

V -100.09

Atmospheric data

Teff 5766
log g 3.9
vturb 1.1

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
O I...-0.58+-0.0690.88+-0.0698.29+-0.069
Na I...-1.53+-0.054-0.07+-0.0544.80+-0.054
Mg I...-0.97+-0.0550.49+-0.0556.61+-0.055
Si I...-1.12+-0.0480.34+-0.0486.43+-0.048
Ca I...-1.07+-0.0330.39+-0.0335.29+-0.033
Ti I...-1.23+-0.030.23+-0.033.79+-0.03
Ti II...-1.09+-0.0480.37+-0.0483.93+-0.048
Fe I...-1.46+-0.051...6.04+-0.051
Fe II...-1.49+-0.066...6.01+-0.066
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)