HD105004
taken from 8 paper(s):
/C.J.Akerman et al.(2004)/
/P.E.Nissen et al.(2004)/
/R.Smiljanic et al.(2009)/
/C.J.Hansen et al.(2012)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/

C.J.Akerman et al.,AAP, 414, 931, 2004 (A0123,ADS)
The evolution of the C/O ratio in metal-poor halo stars
Stellar Parameters
Teff : 5919 | log g : 4.36 | vturb : 1.2 |
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 |
C I | N/A | ... | ... | 7.75 | -0.68 | 0.18 | 7.75 | C I |
O I | N/A | ... | ... | 8.26 | -0.43 | 0.43 | 8.26 | O I |
Fe | N/A | -.86 | ... | ... | -0.86 | ... | 6.64 | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 60000 | 200-300 | 3600 | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P.E.Nissen et al.,AAP, 415, 993, 2004 (A0160,ADS)
Sulphur and zinc abundances in Galactic stars and damped Ly alpha systems
Stellar Parameters
Teff : 5919+-70 | log g : 4.36+-0.15 | vturb : 1.2+-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 |
S I | N/A | -0.85 | ... | ... | -0.77 | 0.09 | 6.35 | S I |
Fe II | N/A | -0.86 | ... | ... | -0.86 | ... | 6.64 | Fe II |
Zn I | N/A | -0.86 | ... | ... | -0.85 | 0.01 | 3.71 | Zn I |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001 | N/A | VLT | 60000 | 150-300 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
R.Smiljanic et al.,AAP, 499, 103, 2009 (A0190,ADS)
Beryllium abundances and star formation in the halo and in the thick disk
Stellar Parameters
Teff : 5831 | log g : 4.36 | 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 |
Li | N/A | ... | ... | 1.95 | -1.31 | -0.51 | 1.95 | Li |
Be | N/A | ... | ... | 0.36 | -1.02 | -0.22 | 0.36 | Be |
Fe | N/A | -0.8 | ... | ... | -0.80 | ... | 6.70 | Fe |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
C.J.Hansen et al.,AAP, 545, A31, 2012 (A0272,ADS)
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
Teff : 5900+-100 | log g : 4.30+-0.25 | vturb : 1.1+-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 |
Fe | N/A | -0.84+-0.15 | ... | ... | -0.84+-0.15 | ... | 6.66+-0.15 | Fe |
Sr | N/A | ... | 0.10+-0.10 | ... | -0.74+-0.10 | 0.10+-0.10 | 2.13+-0.10 | Sr |
Y | N/A | ... | -0.19+-0.12 | ... | -1.03+-0.12 | -0.19+-0.12 | 1.18+-0.12 | Y |
Zr | N/A | ... | 0.02+-0.17 | ... | -0.82+-0.17 | 0.02+-0.17 | 1.76+-0.17 | Zr |
Pd | N/A | ... | 0.12+-0.19 | ... | -0.72+-0.19 | 0.12+-0.19 | 0.85+-0.19 | Pd |
Ag | N/A | ... | 0.01+-0.27 | ... | -1.09+-0.27 | -0.25+-0.27 | 0.11+-0.27 | Ag |
Ba | N/A | ... | 0.17+-0.18 | ... | -0.67+-0.18 | 0.17+-0.18 | 1.51+-0.18 | Ba |
Eu | N/A | ... | 0.26+-0.20 | ... | -0.58+-0.20 | 0.26+-0.20 | -0.06+-0.20 | Eu |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 40000 | >100 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
M.N.Ishigaki et al.,ApJ, 753, 64, 2012 (A0273,ADS)
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. I. Implications of [alpha/Fe] for Star Formation Histories in Their Progenitors
Stellar Parameters
Teff : 6115+-100 | log g : 5.00+-0.3 | vturb : 0.40+-0.3 |
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 |
Mg | N/A | ... | 0.02+-0.09 | ... | -0.56+-0.09 | 0.02+-0.09 | 7.04+-0.09 | Mg |
Si | N/A | ... | 0.04+-0.12 | ... | -0.54+-0.12 | 0.04+-0.12 | 6.97+-0.12 | Si |
Ca | N/A | ... | -0.07+-0.08 | ... | -0.65+-0.08 | -0.07+-0.08 | 5.69+-0.08 | Ca |
Ti I | N/A | ... | 0.19+-0.08 | ... | -0.39+-0.08 | 0.19+-0.08 | 4.56+-0.08 | Ti I |
Ti II | N/A | ... | 0.35+-0.07 | ... | -0.23+-0.07 | 0.35+-0.07 | 4.72+-0.07 | Ti II |
Fe I | N/A | -0.58+-0.12 | ... | ... | -0.58+-0.12 | ... | 6.92+-0.12 | Fe I |
Fe II | N/A | -0.60+-0.10 | ... | ... | -0.60+-0.10 | ... | 6.90+-0.10 | Fe II |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | SUBARUHDS | 50000 | N/A | N/A | 120.9+-0.4 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -263536.09 | Right Ascension : 120525.548 |
M.N.Ishigaki et al.,ApJ, 771, 67, 2013 (A0286,ADS)
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 6115 | log g : 5 | vturb : 0.4 |
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 |
Na I | N/A | ... | -0.09+-0.1 | ... | -0.66+-0.1 | -0.09+-0.1 | 5.58+-0.1 | Na I |
Sc II | N/A | ... | 0.19+-0.07 | ... | -0.38+-0.07 | 0.19+-0.07 | 2.77+-0.07 | Sc II |
V I | N/A | ... | 0.11+-0.2 | ... | -0.46+-0.2 | 0.11+-0.2 | 3.47+-0.2 | V I |
Cr I | N/A | ... | -0.08+-0.07 | ... | -0.65+-0.07 | -0.08+-0.07 | 4.99+-0.07 | Cr I |
Cr II | N/A | ... | 0.15+-0.09 | ... | -0.42+-0.09 | 0.15+-0.09 | 5.22+-0.09 | Cr II |
Mn I | N/A | ... | -0.12+-0.08 | ... | -0.69+-0.08 | -0.12+-0.08 | 4.74+-0.08 | Mn I |
Fe I | N/A | -0.57+-0.11 | ... | ... | -0.57+-0.11 | ... | 6.93+-0.11 | Fe I |
Fe II | N/A | -0.6+-0.11 | ... | ... | -0.60+-0.11 | ... | 6.90+-0.11 | Fe II |
Ni I | N/A | ... | -0.12+-0.09 | ... | -0.69+-0.09 | -0.12+-0.09 | 5.53+-0.09 | Ni I |
Zn I | N/A | ... | 0.01+-0.1 | ... | -0.56+-0.1 | 0.01+-0.1 | 4.00+-0.1 | Zn I |
Y II | N/A | ... | 0.02+-0.08 | ... | -0.55+-0.08 | 0.02+-0.08 | 1.66+-0.08 | Y II |
Ba II | N/A | ... | 0.21+-0.15 | ... | -0.36+-0.15 | 0.21+-0.15 | 1.82+-0.15 | Ba II |
Nd II | N/A | ... | 0.78+-0.13 | ... | 0.21+-0.13 | 0.78+-0.13 | 1.63+-0.13 | Nd II |
Eu II | N/A | ... | 0.37+-0.21 | ... | -0.20+-0.21 | 0.37+-0.21 | 0.32+-0.21 | Eu II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 50000 | N/A | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P.E.Nissen et al.,AAP, 511, L10, 2010 (C0012,ADS)
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5754 | log g : 4.3 | vturb : 1.2 |
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 |
Na | N/A | ... | -0.05 | ... | -0.78 | 0.04 | 5.46 | Na |
Mg | N/A | ... | 0.17 | ... | -0.67 | 0.15 | 6.93 | Mg |
Si | N/A | ... | 0.14 | ... | -0.64 | 0.18 | 6.87 | Si |
Ca | N/A | ... | 0.17 | ... | -0.63 | 0.19 | 5.71 | Ca |
Ti | N/A | ... | 0.07 | ... | -0.68 | 0.14 | 4.27 | Ti |
Cr | N/A | ... | -0.03 | ... | -0.82 | 0.00 | 4.82 | Cr |
Fe | N/A | -0.82 | ... | ... | -0.82 | ... | 6.68 | Fe |
Ni | N/A | ... | -0.06 | ... | -0.85 | -0.03 | 5.37 | Ni |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-01-12-0732 | N/A | VLT | 55000 | 500 | N/A | 121.8 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P. E. Nissen et al.,AAP, 530, A15, 2011 (C0013,ADS)
Two distinct halo populations in the solar neighborhood II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
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 |
Mn | N/A | ... | -0.21 | ... | -1.07 | -0.25 | 4.36 | Mn |
Fe | N/A | -0.82 | ... | ... | -0.82 | ... | 6.68 | Fe |
Cu | N/A | ... | -0.22 | ... | -1.02 | -0.20 | 3.17 | Cu |
Zn | N/A | ... | 0.04 | ... | -0.74 | 0.08 | 3.82 | Zn |
Y | N/A | ... | -0.15 | ... | -0.94 | -0.12 | 1.27 | Y |
Ba | N/A | ... | -0.16 | ... | -1.03 | -0.21 | 1.15 | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-01-12-0732 | N/A | VLT | 55000 | 500 | N/A | 121.8 |