HD082590: found in 2 paper(s).

Labels:

/J.Simmerer et al.(2004)/ /B.W.Carney et al.(2003)/

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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 6005
log g 2.75
vturb 3.00

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
C...-2.37-1.056.18
Fe II...-1.32...6.18
La II...-1.28+-0.020.04+-0.02-0.11+-0.02
Eu II...-0.97+-0.060.35+-0.06-0.46+-0.06
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

A0138

Title Spectroscopic Binaries, Velocity Jitter, and Rotation in Field Metal-poor Red Giant and Red Horizontal-Branch Stars
ADS B.W.Carney et al.,AJ, 125, 293, 2003
Authors B. W. Carney, D. W. Latham, R. P. Stefanik, J. B. Laird, J. A. Morse

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
N/A 2445689.84469 WYETH N/A N/A N/A 214.19+-0.93
N/A 2445715.76261 WYETH N/A N/A N/A 215.01+-0.64
N/A 2446075.76887 WYETH N/A N/A N/A 215.29+-0.71
N/A 2446131.62615 WYETH N/A N/A N/A 215.73+-1.08
N/A 2446429.83658 WYETH N/A N/A N/A 214.28+-0.97
N/A 2446834.72266 WYETH N/A N/A N/A 214.48+-0.77
N/A 2447138.91268 WYETH N/A N/A N/A 213.78+-1.91
N/A 2447488.93164 WYETH N/A N/A N/A 213.40+-0.91
N/A 2447905.75722 WYETH N/A N/A N/A 213.96+-1.27
N/A 2448286.86327 MMT N/A N/A N/A 215.63+-0.51
N/A 2448638.91438 TILLINGHAST N/A N/A N/A 213.75+-0.74
N/A 2448669.83402 TILLINGHAST N/A N/A N/A 213.58+-0.80
N/A 2448721.59417 WYETH N/A N/A N/A 214.65+-0.80
N/A 2450553.58949 WYETH N/A N/A N/A 213.90+-0.95
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination -172608
Right Ascension 093230.3

Binarity

Vrad 214.40

Photometric data

V-R 0.511
V-K 1.49

Atmospheric data

Teff 5960
log g 2.7

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe...-1.85...5.65
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)