HD233891: found in 3 paper(s).

Labels:

/D.L.Burris et al.(2000)/ /J.P.Fulbright et al.(2003)/ /J.Simmerer et al.(2004)/

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A0014

Title NEUTRON-CAPTURE ELEMENTS IN THE EARLY GALAXY: INSIGHTS FROM A LARGE SAMPLE OF METAL-POOR GIANTS
ADS D.L.Burris et al.,ApJ, 544, 302, 2000
Authors D. L. Burris, C. A. Pilachowski, T. E. Armandroff, C. Sneden, J. J. Cowan, H. Roe

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A N/A MAYALLKPNO 20000 100-200 N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Atmospheric data

Teff 4750
log g 1.60
vturb 2.00

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe...-1.58...5.92
Ba...-1.430.150.70
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

A0074

Title Oxygen Abundances in Metal-poor Stars
ADS J.P.Fulbright et al.,ApJ, 595, 1154, 2003
Authors J. P. Fulbright, J. A. Johnson

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2001-04-06 N/A GECKOCFHT 130000 110 900 N/A
2001-05-05 N/A LICKHAMILTON N/A 70 1800 N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Photometric data

V 8.8
B-V 0.8
V-R 0.72
V-K 2.21

Atmospheric data

Teff 4825
log g 1.91
vturb 1.9

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
O I...-0.75+-0.060.56+-0.067.94+-0.09
Fe...-1.31...6.19
Fe I...-1.49+-0.05...6.01+-0.05
Fe II...-1.29+-0.06...6.21+-0.06
    : 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

Atmospheric data

Teff 4911
log g 2.10
vturb 2.05

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
C...-1.70-0.36.85
Fe I...-1.40...6.10
Fe II...-1.34...6.16
La II...-1.30+-0.060.10+-0.06-0.13+-0.06
Eu II...-1.02+-0.090.38+-0.09-0.51+-0.09
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)