HD36702: found in 2 paper(s).

Labels:

/R.G.Gratton et al.(2000)/ /B.W.Carney et al.(2003)/

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A0049

Title Mixing along the red giant branch in metal-poor field stars
ADS R.G.Gratton et al.,AAP, 354, 169, 2000
Authors R. G. Gratton, C. Sneden, E. Carretta, A. Bragaglia

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
1995-05 N/A CESESO 50000 80-150 N/A N/A
1995-11 N/A CESESO 50000 80-150 N/A N/A
1995-11 N/A MCDONALD 60000 70-100 N/A N/A
Galactic Longitude (l) 243.45
Galactic Latitude (b) -31.40
Declination -383324
Right Ascension 053152.2

Photometric data

V 8.36
B-V 1.215

Atmospheric data

Teff 4366
log g 0.95
vturb 1.65

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Li I...-1.160.900.00
O I...-1.660.407.21
Na...-2.30-0.244.03
Fe I...-2.06...5.44
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

Isotope ratio

12C/13C 10

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 2446016.88504 TILLINGHAST N/A N/A N/A 122.20+-0.39
N/A 2446452.71381 MMT N/A N/A N/A 122.07+-0.40
N/A 2446512.60680 MMT N/A N/A N/A 122.81+-0.39
N/A 2446867.59728 TILLINGHAST N/A N/A N/A 123.09+-0.41
N/A 2447136.87902 TILLINGHAST N/A N/A N/A 123.01+-0.41
N/A 2447465.95745 TILLINGHAST N/A N/A N/A 122.76+-0.35
N/A 2447847.91769 TILLINGHAST N/A N/A N/A 121.33+-0.39
N/A 2448525.03646 MMT N/A N/A N/A 122.48+-0.52
N/A 2448526.02640 MMT N/A N/A N/A 123.01+-0.34
N/A 2449373.76897 MMT N/A N/A N/A 123.45+-0.46
N/A 2450822.70866 MMT N/A N/A N/A 123.56+-0.34
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination -383324
Right Ascension 053152.1

Binarity

Vrad 122.71

Photometric data

Atmospheric data

Teff 4180
log g 0.8

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
Fe...-1.86...5.64
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)