HE1305+0007: found in 2 paper(s).

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/A.Goswami et al.(2006)/ /T.C.Beers et al.(2007)/

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A0094

Title A high-resolution spectral analysis of three carbon-enhanced metal-poor stars
ADS A.Goswami et al.,MNRAS, 372, 343, 2006
Authors A. Goswami, W. Aoki, T. C. Beers, N. Christlieb, J. E. Norris, S. G. Ryan, S. Tsangarides

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2003-3-25 2452784.95121 SUBARUHDS 50000 N/A 600 N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination
Right Ascension

Photometric data

V 12.22
B-V 1.459
V-R 0.682
H 9.753
J 10.247
K 9.600
EB-V 0.038

Atmospheric data

Teff 4750
log g 2.0
vturb 2.0

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
C I...-0.191.848.2
Na I...-1.77+0.264.40
Mg I...-1.780.255.75
Ca I...-1.90.134.41
Sc II...-1.90.091.15
Ti II...-1.20.793.7
Mn I...-1.890.143.5
Fe I...-2.03...5.42+-0.18
Fe II...-1.99...5.46+-0.17
Ni I...-2.28-0.253.95
Sr I...-1.170.861.75
Y II...-1.260.730.95
Ba II...0.332.322.5
La II...0.572.561.7
Ce II...0.542.532.12
Pr II...0.392.381.1
Nd II...0.62.592.05
Sm II...0.612.61.62
Eu II...-0.021.970.5
Pb I...0.382.372.38
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)


A0111

Title NEAR-INFRARED SPECTROSCOPY OF CARBON-ENHANCED METAL-POOR STARS. I. A SOAR /OSIRIS PILOT STUDY
ADS T.C.Beers et al.,AJ, 133, 1193, 2007
Authors T. C. Beers, T. Sivarani, B. Marsteller, Y. S. Lee, S. Rossi, B. Plez

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Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2006-01-18 N/A SOAROSIRIS 3000 60 1800 N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Photometric data

V 12.223
B-V 1.459
V-R 0.682
H 9.753
J 10.247
K 9.600
EB-V 0.022

Atmospheric data

Teff 4560
log g 1.0

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
C...-0.10+-0.35+2.4+-0.358.45+-0.35
N...-0.60+-0.46+1.9+-0.467.37+-0.46
O...-1.70+-0.22+0.8+-0.227.17+-0.22
Fe...-2.5...5.00
Ba...0.40+-0.5+2.9+-0.52.53+-0.5
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)

Isotope ratio

12C/13C 9+-2