BPS CS29493-090: found in 2 paper(s).

Labels:

/P.S.Barklem et al.(2005)/ /J.A.Johnson et al.(2007)/

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A0052

Title The Hamburg/ESO R-process enhanced star survey (HERES). II. Spectroscopic analysis of the survey sample
ADS P.S.Barklem et al.,AAP, 439, 129, 2005
Authors P. S. Barklem, N. Christlieb, T. C. Beers, V. Hill, M. S. Bessell, J. Holmberg, B. Marsteller, S. Rossi, F. -J. Zickgraf, D. Reimers

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A VLT 20000 60 N/A 269.8

Photometric data

V 14.07

Atmospheric data

Teff 4692
log g 1.28
vturb 1.93

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
CH...-2.55+-0.270.74+-0.296.00+-0.27
Mg I...-2.36+-0.240.77+-0.245.22+-0.19
Al I...-3.20+-0.25-0.07+-0.273.27+-0.25
Ca I...-2.83+-0.200.31+-0.253.53+-0.20
Sc II...-2.74+-0.250.39+-0.250.42+-0.24
Ti...-2.97+-0.220.16+-0.222.05+-0.20
Cr I...-3.50+-0.26-0.37+-0.262.17+-0.26
Mn I...-3.68+-0.26-0.55+-0.261.71+-0.23
Fe...-3.13+-0.180.00+-0.224.37+-0.18
Co I...-2.88+-0.220.26+-0.242.04+-0.22
Ni I...-3.34+-0.26-0.21+-0.262.91+-0.26
Sr...-4.02+-0.29-0.89+-0.29-1.06+-0.30
Y II...-4.03+-0.25-0.90+-0.25-1.79+-0.24
Ba II...-2.61+-0.310.52+-0.29-0.48+-0.31
La II...-2.81+-0.240.32+-0.24-1.64+-0.22
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0114

Title A Search for Nitrogen-enhanced Metal-poor Stars
ADS J.A.Johnson et al.,ApJ, 658, 1203, 2007
Authors J. A. Johnson, F. Herwig, T. C. Beers, N. Christlieb

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2003-09-04 N/A RCCTIO N/A 57 3600 N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Photometric data

V 14.039
B-V 0.835
V-R 0.516
V-K 2.366
EB-V 0.03

Atmospheric data

Teff 4739
log g 1.56
vturb 1.97

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
C...-2.57+-0.29+0.25+-0.295.99+-0.25
N...-2.37+-0.25+0.45+-0.255.68+-0.25
Fe...-2.82+-0.21...4.68+-0.21
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)