G5-19

taken from 8 paper(s):

/R.Smiljanic et al.(2009)/ /A.M.Boesgaard et al.(2005)/ /A.Stephens and A. M. Boesgaard(2002)/ /H.L.Yan et al.(2016)/ /A.M.Boesgaard et al.(2011)/ /K.A.Venn et al.(2004)/ /P.E.Nissen and W. J. Schuster(2010)/ /P. E. Nissen and W. J. Schuster(2011)/


R.Smiljanic et al.,AAP, 499, 103, 2009(ADS)

Beryllium abundances and star formation in the halo and in the thick disk


Stellar Parameters

Teff : 5942 log g : 4.24 vturb : 0.89

Chemical Abundances

Original Data Converted Data Asplund et al. (2009)
Element Nline [X/H] [X/Fe] log-e [X/H] [X/Fe] log-e Element
LiN/A......2.26-1.000.102.26Li
BeN/A......-0.01-1.39-0.29-0.01Be
FeN/A-1.1......-1.10...6.40Fe


A.M.Boesgaard et al.,ApJ, 633, 398, 2005(ADS)

Lithium and Lithium Depletion in Halo Stars on Extreme Orbits


Stellar Parameters

Teff : 5942+-56 log g : 4.24+-0.24 vturb : 0.89+-0.11

Chemical Abundances

Original Data Converted Data Asplund et al. (2009)
Element Nline [X/H] [X/Fe] log-e [X/H] [X/Fe] log-e Element
Li IN/A......2.26+-0.05-1.00+-0.050.08+-0.052.26+-0.05Li I
FeN/A-1.10+-0.08......-1.08+-0.08...6.42+-0.08Fe

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
N/A KECKHIRES 48000 110 N/A N/A

A.Stephens et al.,AJ, 123, 1647, 2002(ADS)

ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS


Stellar Parameters

Teff : 5942+-56 log g : 4.24+-0.24 vturb : 0.89+-0.11

Chemical Abundances

Original Data Converted Data Asplund et al. (2009)
Element Nline [X/H] [X/Fe] log-e [X/H] [X/Fe] log-e Element
Na IN/A-1.37+-0.20-0.21+-0.20...-1.28+-0.20-0.13+-0.204.96+-0.20Na I
Mg IN/A-0.96+-0.09+0.20+-0.10...-0.98+-0.090.17+-0.106.62+-0.09Mg I
SiN/A...+0.12+-0.10...-1.00+-0.100.15+-0.106.51+-0.10Si
Si I3-0.97+-0.12......-0.93+-0.120.22+-0.126.58+-0.12Si I
Si II1-1.17+-0.16......-1.13+-0.160.02+-0.166.38+-0.16Si II
Ca IN/A-0.97+-0.08+0.19+-0.09...-0.95+-0.080.20+-0.095.39+-0.08Ca I
TiN/A...+0.22+-0.09...-0.90+-0.090.25+-0.094.05+-0.09Ti
Ti I16-1.00+-0.12......-0.96+-0.120.19+-0.123.99+-0.12Ti I
Ti II8-0.90+-0.10......-0.86+-0.100.29+-0.104.09+-0.10Ti II
CrN/A...+0.00+-0.08...-1.13+-0.080.02+-0.084.51+-0.08Cr
Cr I14-1.18+-0.08......-1.15+-0.080.00+-0.084.49+-0.08Cr I
Cr II5-1.06+-0.17......-1.03+-0.170.12+-0.174.61+-0.17Cr II
FeN/A-1.16+-0.04......-1.15+-0.04...6.35+-0.04Fe
Fe I71-1.09+-0.08......-1.08+-0.08...6.42+-0.08Fe I
Fe II10-1.18+-0.05......-1.17+-0.05...6.33+-0.05Fe II
Ni IN/A-1.26+-0.13-0.10+-0.13...-1.23+-0.13-0.08+-0.134.99+-0.13Ni I
Y IIN/A-1.21+-0.05-0.05+-0.07...-1.18+-0.05-0.03+-0.071.03+-0.05Y II
Ba IIN/A-1.01+-0.13+0.15+-0.14...-1.06+-0.130.09+-0.141.12+-0.13Ba II

Binary Parameters

Vrad -215.6+-0.6

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2451067.648 KECKHIRES 48000 110 200 -215.6+-0.6

H.L.Yan et al.,AAP, 585, 102, 2016(ADS)

Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood


Stellar Parameters

Teff : 5854 log g : 4.26 vturb : 1.3

Chemical Abundances

Original Data Converted Data Asplund et al. (2009)
Element Nline [X/H] [X/Fe] log-e [X/H] [X/Fe] log-e Element
FeN/A-1.18......-1.18...6.32Fe
CuN/A...-0.70+-0.00...-1.86+-0.00-0.68+-0.002.33+-0.00Cu

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
N/A VLT 55000 250-500 N/A N/A

A.M.Boesgaard et al.,ApJ, 743, 140, 2011(ADS)

Beryllium and Alpha-element Abundances in a Large Sample of Metal-poor Stars


Stellar Parameters

Teff : 5975+-100 log g : 3.93+-0.2 vturb : 1.34+-0.2

Chemical Abundances

Original Data Converted Data Asplund et al. (2009)
Element Nline [X/H] [X/Fe] log-e [X/H] [X/Fe] log-e Element
BeN/A...-0.37+-0.15-0.08+-0.12-1.46+-0.12-0.33+-0.15-0.08+-0.12Be
ON/A-0.62+-0.22+0.51+-0.24...-0.68+-0.220.45+-0.248.01+-0.22O
MgN/A-0.88+-0.07......-0.90+-0.070.23+-0.076.70+-0.07Mg
TiN/A-1.02+-0.09......-0.95+-0.090.18+-0.094.00+-0.09Ti
FeN/A-1.13+-0.09......-1.13+-0.09...6.37+-0.09Fe

Position

Right Ascension : Declination : Galactic Longitude (l) : N/A Galactic Latitude (b) : N/A

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2005-09-27 N/A KECKHIRES 42000 90 3600 N/A

K.A.Venn et al.,AJ, 128, 1177, 2004(ADS)

Stellar Chemical Signatures and Hierarchical Galaxy Formation


Chemical Abundances

Original Data Converted Data Asplund et al. (2009)
Element Nline [X/H] [X/Fe] log-e [X/H] [X/Fe] log-e Element
NaN/A...-0.21...-1.28-0.124.96Na
MgN/A...0.2...-0.980.186.62Mg
CaN/A...0.19...-0.950.215.39Ca
TiN/A...0.22...-0.870.294.08Ti
FeN/A-1.16......-1.16...6.34Fe
NiN/A...-0.1...-1.23-0.074.99Ni
YN/A...-0.14...-1.27-0.110.94Y
BaN/A...0.15...-1.060.101.12Ba


P.E.Nissen et al.,AAP, 511, L10, 2010(ADS)

Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics


Stellar Parameters

Teff : 5854 log g : 4.26 vturb : 1.3

Chemical Abundances

Original Data Converted Data Asplund et al. (2009)
Element Nline [X/H] [X/Fe] log-e [X/H] [X/Fe] log-e Element
NaN/A...-0.25...-1.34-0.164.90Na
MgN/A...0.18...-1.020.166.58Mg
SiN/A...0.17...-0.970.216.54Si
CaN/A...0.26...-0.900.285.44Ca
TiN/A...0.14...-0.970.213.98Ti
CrN/A...-0.05...-1.20-0.024.44Cr
FeN/A-1.18......-1.18...6.32Fe
NiN/A...-0.13...-1.28-0.104.94Ni

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2005-10-15-0521 N/A VLT 55000 300 N/A -216.2

P. E. Nissen et al.,AAP, 530, A15, 2011(ADS)

Two distinct halo populations in the solar neighborhood II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba


Stellar Parameters

Teff : 5854 log g : 4.26

Chemical Abundances

Original Data Converted Data Asplund et al. (2009)
Element Nline [X/H] [X/Fe] log-e [X/H] [X/Fe] log-e Element
MnN/A...-0.35...-1.57-0.393.86Mn
FeN/A-1.18......-1.18...6.32Fe
CuN/A...-0.62...-1.78-0.602.41Cu
ZnN/A...0.01...-1.130.053.43Zn
YN/A...-0.12...-1.27-0.090.94Y
BaN/A...-0.17...-1.40-0.220.78Ba

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2005-10-15-0521 N/A VLT 55000 300 N/A -216.2