BD+28_2137: found in 2 paper(s).

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/G.S.Bai et al.(2004)/ /P.E.Niseen et al.(2007)/

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A0023

Title Chemical abundances of 10 metal-poor halo stars
ADS G.S.Bai et al.,AAP, 425, 671, 2004
Authors G. S. National Astronomical Observatories, ChineseAcademyofSciencea. Bai, G. Zhao, Y. Q. National Astronomical Observatories, ChineseAcademyofSciencea. Chen, J. R. National Astronomical Observatories, ChineseAcademyofSciencea. Shi, V. G. Special Astrophysical Observatory, RussianAcademyofSciences. Klochkova, V. E. Special Astrophysical Observatory, RussianAcademyofSciences. Panchuk, H. M. National Astronomical Observatories, ChineseAcademyofSciencea. Qiu, H. W. National Astronomical Observatories, ChineseAcademyofSciencea. Zhang

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2001-04-23 N/A PFESSAO 15000 240 N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Photometric data

V 10.89

Atmospheric data

Teff 6135
log g 4.25+-0.3
vturb 1.50

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
O I...-1.370.567.50
Na I...-2.27-0.344.06
Mg I...-1.720.215.86
Si I...-1.450.486.10
Ca I...-1.590.344.77
Sc II...-1.780.151.39
Ti...-1.500.433.52
Cr...-1.920.013.75
Mn I...-2.16-0.233.23
Fe I...-1.93...5.57
Ba II...-1.900.030.23
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0119

Title Sulphur and zinc abundances in Galactic halo stars revisited
ADS P.E.Niseen et al.,AAP, 469, 319, 2007
Authors P. E. Niseen, C. Ackerman, M. Asplund, D. Fabbian, F. Kerber, H. U. Kaufl, M. Pettini

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2007-06-25 N/A VLT 60000 N/A N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Photometric data

V 10.892
K 9.560

Atmospheric data

Teff 6272
log g 4.23
vturb 1.5

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
S I...-1.630.305.70
Fe...-1.93...5.57
Zn I...-1.870.062.73
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)