G 75-31: found in 3 paper(s).

Labels:

/P.E.Nissen et al.(2002)/ /M.Asplund et al.(2006)/ /E.Caffau et al.(2005)/

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A0048

Title O/Fe in metal-poor main sequence and subgiant stars
ADS P.E.Nissen et al.,AAP, 390, 235, 2002
Authors P. E. Nissen, F. Primas, M. Asplund, D. L. Lambert

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2000-04 N/A VLT 55000 300-400 N/A N/A

Photometric data

V 10.53

Atmospheric data

Teff 5952
log g 4.07
vturb 1.3

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
O I...-0.89+0.11-0.150.15+0.11-0.157.98+0.11-0.15
Fe...-1.04...6.46
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

A0089

Title Lithium Isotopic Abundances in Metal-poor Halo Stars
ADS M.Asplund et al.,ApJ, 644, 229, 2006
Authors M. Asplund, D. L. Lambert, P. E. Nissen, F. Primas, V. V. Smith

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2000-07-24-0946 N/A VLT 120000 500 60 57.8
2000-08-04-0926 N/A VLT 120000 500 60 57.8
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Binarity

Vrad 57.8

Photometric data

V 10.52

Atmospheric data

Teff 6000
log g 4.08
vturb 1.3

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li...1.14+-0.012.16+-0.012.30+-0.01
O...-0.680.348.19
Fe...-1.02...6.48
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

Isotope ratio

6Li/7Li 0.015+-0.012

A0137

Title Sulphur abundance in Galactic stars
ADS E.Caffau et al.,AAP, 441, 533, 2005
Authors E. Caffau, P. Bonifacio, R. Faraggiana, P. Francois, R. G. Gratton, M. Barbieri

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A 2450671.91451 EMMIESO 60000 120 N/A
N/A 2450671.87569 EMMIESO 60000 120 N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination 22644
Right Ascension 23822

Binarity

Vrad 57

Atmospheric data

Teff 5884
log g 4.24

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
S I...-0.73+-0.140.52+-0.146.60+-0.14
Fe...-1.25...6.25
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)