BD+51_1696: found in 2 paper(s).

Labels:

/G.S.Bai et al.(2004)/ /J.Simmerer et al.(2004)/

Find this object in SIMBAD


A0023

Title Chemical abundances of 10 metal-poor halo stars
ADS G.S.Bai et al.,AAP, 425, 671, 2004
Authors G. S. National Astronomical Observatories, ChineseAcademyofSciencea. Bai, G. Zhao, Y. Q. National Astronomical Observatories, ChineseAcademyofSciencea. Chen, J. R. National Astronomical Observatories, ChineseAcademyofSciencea. Shi, V. G. Special Astrophysical Observatory, RussianAcademyofSciences. Klochkova, V. E. Special Astrophysical Observatory, RussianAcademyofSciences. Panchuk, H. M. National Astronomical Observatories, ChineseAcademyofSciencea. Qiu, H. W. National Astronomical Observatories, ChineseAcademyofSciencea. Zhang

Get more information of this paper.

Basic Informations

Observation Date JD Facility Resolution S/N Exposure Time Vrad
2001-04-21 N/A PFESSAO 15000 170 N/A N/A
Galactic Longitude (l) N/A
Galactic Latitude (b) N/A
Declination N/A
Right Ascension N/A

Photometric data

V 9.91

Atmospheric data

Teff 5537
log g 4.55+-0.3
vturb 1.60

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
O I...-0.950.537.92
Na I...-2.09-0.614.24
Mg I...-1.300.186.28
Si I...-1.130.356.42
Ca I...-1.190.295.17
Sc II...-1.330.151.84
Ti...-1.180.303.84
Cr...-1.440.044.23
Mn I...-1.68-0.203.71
Fe I...-1.48...6.02
Ba II...-1.400.080.73
    : 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

Get more information of this paper.

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 5593
log g 4.50
vturb 1.20

Chemical Abundances

Element Nline [X/H] [X/Fe] log-e
C...-1.39-0.057.16
Fe I...-1.34...6.16
Fe II...-1.39...6.11
La II...-1.25+-0.040.09+-0.04-0.08+-0.04
Eu II...-0.83+-0.040.51+-0.04-0.32+-0.04
    : Data presented in the paper
    : Data converted with the solar abundance from Grevesse et al. (1996)