HD3567

taken from 12 paper(s):

/P.E.Nissen et al.(2002)/ /T.V.Mishenina et al.(2002)/ /T.V.Mishenina and V. V. Kovtyukh(2001)/ /M.Asplund et al.(2006)/ /J.P.Fulbright(2000)/ /R.G.Gratton et al.(2003)/ /R.Smiljanic et al.(2009)/ /C.J.Hansen et al.(2012)/ /H.L.Yan et al.(2016)/ /B.E.Reddy et al.(2006)/ /P.E.Nissen and W. J. Schuster(2010)/ /P. E. Nissen and W. J. Schuster(2011)/


P.E.Nissen et al.,AAP, 390, 235, 2002(ADS)

O/Fe in metal-poor main sequence and subgiant stars


Stellar Parameters

Teff : 6000 log g : 4.07 vturb : 1.5

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
[O I]N/A...0.42+0.08-0.108.00+0.08-0.10-0.69+0.08-0.100.44+0.08-0.108.00+0.08-0.10[O I]
FeN/A-1.16......-1.13...6.37Fe

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2000-04 N/A VLT 55000 300-400 N/A N/A

T.V.Mishenina et al.,AAP, 396, 189, 2002(ADS)

Abundances of Cu and Zn in metal-poor stars: Clues for Galaxy evolution


Stellar Parameters

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-1.2......-1.20...6.30Fe
Cu IN/A...-0.66+-0.13...-1.84+-0.13-0.64+-0.132.35+-0.13Cu I
Zn IN/A...-0.23+-0.16...-1.39+-0.16-0.19+-0.163.17+-0.16Zn I

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
N/A N/A ELODIE 42000 >100 N/A N/A

T.V.Mishenina et al.,AAP, 370, 951, 2001(ADS)

Analysis of neutron capture elements in metal-poor stars


Stellar Parameters

Teff : 5950 log g : 3.8 vturb : 0.5

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
Mg IN/A...-0.06...-1.28-0.086.32Mg I
Si IN/A...0.21...-0.950.256.56Si I
Ca IN/A...0.41...-0.770.435.57Ca I
FeN/A-1.20......-1.20...6.30Fe
Sr IN/A...0.37...-0.730.472.14Sr I
Ba IIN/A...0.27...-0.980.221.20Ba II
Ce IIN/A...0.23...-0.970.230.61Ce II
Nd IIN/A...0.30...-0.820.380.60Nd II

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
N/A N/A ELODIE 42000 >100 N/A N/A

M.Asplund et al.,ApJ, 644, 229, 2006(ADS)

Lithium Isotopic Abundances in Metal-poor Halo Stars


Stellar Parameters

Teff : 6026 log g : 4.08 vturb : 1.5

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......2.32+-0.01-0.94+-0.010.20+-0.012.32+-0.01Li
ON/A-0.79......-0.740.407.95O
FeN/A-1.14......-1.14...6.36Fe

Isotopic Ratio

6Li/7Li 0.017+-0.012

Binary Parameters

Vrad -47.3

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2000-07-24-0843 N/A VLT 120000 560 45 -47.3

J.P.Fulbright et al.,AJ, 120, 1841, 2000(ADS)

ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS


Stellar Parameters

Teff : 5950 log g : 3.9 vturb : 1.4

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......2.3-0.960.342.3Li I
Na IN/A...-0.17...-1.40-0.104.84Na I
Mg IN/A...0.27...-1.070.236.53Mg I
Si IN/A...0.34...-0.940.366.57Si I
Ca IN/A...0.33...-0.970.335.37Ca I
TiN/A...0.31...-0.970.333.98Ti
V IN/A...0.09...-1.160.142.77V I
Cr IN/A...-0.01...-1.300.004.34Cr I
FeN/A-1.32......-1.30...6.20Fe
Ni IN/A...-0.05...-1.34-0.044.88Ni I
Y IIN/A...-0.06...-1.35-0.050.86Y II
Zr IIN/A...0.23...-1.070.231.51Zr II
Ba IIN/A...0.15...-1.220.080.96Ba II

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
1998-08-08 N/A LICKHAMILTON 50000 120 1800 N/A

R.G.Gratton et al.,AAP, 404, 187, 2003(ADS)

Abundances for metal-poor stars with accurate parallaxes I. Basic data


Stellar Parameters

Teff : 6087 log g : 4.16 vturb : 0.98

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
O IN/A...0.46+-0.069...-0.69+-0.0690.54+-0.0698.00+-0.069O I
Na IN/A...-0.28+-0.054...-1.53+-0.054-0.30+-0.0544.71+-0.054Na I
Mg IN/A...0.22+-0.055...-1.17+-0.0550.06+-0.0556.43+-0.055Mg I
Si IN/A...0.17+-0.048...-1.03+-0.0480.20+-0.0486.48+-0.048Si I
Ca IN/A...0.32+-0.033...-0.97+-0.0330.26+-0.0335.37+-0.033Ca I
Ti IN/A...0.17+-0.03...-0.93+-0.030.30+-0.034.02+-0.03Ti I
Ti IIN/A...0.27+-0.048...-0.83+-0.0480.40+-0.0484.12+-0.048Ti II
Fe IN/A-1.22+-0.051......-1.23+-0.051...6.27+-0.051Fe I
Fe IIN/A-1.26+-0.066......-1.27+-0.066...6.23+-0.066Fe II

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
N/A VLT 50000 200 N/A -49.7

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 : 5950 log g : 4.1 vturb : 1.4

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......2.42-0.840.362.42Li
BeN/A......-0.11-1.49-0.29-0.11Be
FeN/A-1.2......-1.20...6.30Fe


C.J.Hansen et al.,AAP, 545, A31, 2012(ADS)

Silver and palladium help unveil the nature of a second r-process


Stellar Parameters

Teff : 6035+-100 log g : 4.08+-0.25 vturb : 1.5+-0.15

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-1.33+-0.15......-1.33+-0.15...6.17+-0.15Fe
SrN/A...-0.1+-0.20...-1.43+-0.20-0.10+-0.201.44+-0.20Sr
YN/A...-0.18+-0.19...-1.51+-0.19-0.18+-0.190.70+-0.19Y
ZrN/A...0.27+-0.17...-1.06+-0.170.27+-0.171.52+-0.17Zr
PdN/A...0.29+-0.20...-1.04+-0.200.29+-0.200.53+-0.20Pd
AgN/A...0.53+-0.25...-1.06+-0.250.27+-0.250.14+-0.25Ag
BaN/A...0.26+-0.17...-1.07+-0.170.26+-0.171.11+-0.17Ba
EuN/A...0.70+-0.18...-0.63+-0.180.70+-0.18-0.11+-0.18Eu

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
N/A VLT 40000 >100 N/A N/A

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 : 6051 log g : 4.02 vturb : 1.5

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-1.16......-1.16...6.34Fe
CuN/A...-0.73+-0.00...-1.87+-0.00-0.71+-0.002.32+-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

B.E.Reddy et al.,MNRAS, 367, 1329, 2006(ADS)

Elemental abundance survey of the Galactic thick disc


Stellar Parameters

Teff : 6060 log g : 4.47

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
ON/A...0.47...-0.530.568.16O
NaN/A...0.07...-0.940.155.30Na
MgN/A...0.19...-0.910.186.69Mg
SiN/A...0.09...-0.840.256.67Si
CaN/A...0.11...-0.940.155.40Ca
ScN/A...0.13...-0.820.272.33Sc
TiN/A...0.2...-0.890.204.06Ti
CrN/A...-0.21...-1.21-0.124.43Cr
MnN/A...-0.52...-1.62-0.533.81Mn
Fe IN/A-1.04......-1.09...6.41Fe I
CoN/A...0.31...-0.790.304.20Co
NiN/A...-0.01...-1.040.055.18Ni
ZnN/A...0.03...-1.10-0.013.46Zn
YN/A...0.06...-1.070.021.14Y
BaN/A...0.09...-0.930.161.25Ba

Binary Parameters

Vrad -50.2

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2004-06 N/A MCDONALD 60000 100-200 N/A -50.2

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 : 6051 log g : 4.02 vturb : 1.5

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...-0.24...-1.31-0.154.93Na
MgN/A...0.14...-1.040.126.56Mg
SiN/A...0.17...-0.950.216.56Si
CaN/A...0.31...-0.830.335.51Ca
TiN/A...0.22...-0.870.294.08Ti
CrN/A...-0.05...-1.18-0.024.46Cr
FeN/A-1.16......-1.16...6.34Fe
NiN/A...-0.13...-1.26-0.104.96Ni

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2001-10-08-0419 N/A VLT 55000 650 N/A -47.8

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 : 6051 log g : 4.02

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...-0.33...-1.53-0.373.90Mn
FeN/A-1.16......-1.16...6.34Fe
CuN/A...-0.72...-1.86-0.702.33Cu
ZnN/A...0.01...-1.110.053.45Zn
YN/A...-0.05...-1.18-0.021.03Y
BaN/A...-0.09...-1.30-0.140.88Ba

Position

Observing Log

Date of Observation JD Facility Resolution S/N Exposure Time Vrad
2001-10-08-0419 N/A VLT 55000 650 N/A -47.8