HD22879
Original Names
BD-03_592 in E.Caffau+,AAP, 441, 533, 2005HIP17147 in T.Bensby+,AAP, 433, 185, 2005
taken from 15 paper(s):
/J.P.Fulbright(2000)/
/J.Simmerer et al.(2004)/
/R.G.Gratton et al.(2003)/
/G.Bihain et al.(2004)/
/G.Israelian et al.(1998)/
/R.Smiljanic et al.(2009)/
/T.Gehren et al.(2006)/
/C.J.Hansen et al.(2012)/
/H.L.Yan et al.(2016)/
/T.Mishenina et al.(2017)/
/B.E.Reddy et al.(2006)/
/T.V.Mishenina et al.(2013)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
/T.Mishenina et al.(2019)/
ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
Stellar Parameters
Teff : 5800 | log g : 4.3 | vturb : 1.1 |
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 I | N/A | ... | ... | 1.44 | -1.82 | -0.93 | 1.44 | Li I |
Na I | N/A | ... | 0.08 | ... | -0.74 | 0.15 | 5.50 | Na I |
Mg I | N/A | ... | 0.41 | ... | -0.52 | 0.37 | 7.08 | Mg I |
Al I | N/A | ... | 0.31 | ... | -0.58 | 0.31 | 5.87 | Al I |
Si I | N/A | ... | 0.35 | ... | -0.52 | 0.37 | 6.99 | Si I |
Ca I | N/A | ... | 0.26 | ... | -0.63 | 0.26 | 5.71 | Ca I |
Ti | N/A | ... | 0.32 | ... | -0.55 | 0.34 | 4.40 | Ti |
V I | N/A | ... | 0.18 | ... | -0.66 | 0.23 | 3.27 | V I |
Cr I | N/A | ... | 0.03 | ... | -0.85 | 0.04 | 4.79 | Cr I |
Fe | N/A | -0.91 | ... | ... | -0.89 | ... | 6.61 | Fe |
Ni I | N/A | ... | 0.02 | ... | -0.86 | 0.03 | 5.36 | Ni I |
Y II | N/A | ... | 0.05 | ... | -0.83 | 0.06 | 1.38 | Y II |
Zr II | N/A | ... | 0.27 | ... | -0.62 | 0.27 | 1.96 | Zr II |
Ba II | N/A | ... | 0.11 | ... | -0.85 | 0.04 | 1.33 | Ba II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1994-11-12 | N/A | LICKHAMILTON | 50000 | 145 | 1200 | N/A |
1998-10-30 | N/A | LICKHAMILTON | 50000 | 155 | 600 | N/A |
19990126-31 | N/A | SANDIFORD | 50000 | 100 | 1200 | N/A |
The Rise of the s-Process in the Galaxy
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 I | N/A | -0.91 | ... | ... | -0.91 | ... | 6.59 | Fe I |
Fe II | N/A | -1.03 | ... | ... | -1.03 | ... | 6.47 | Fe II |
La II | N/A | ... | ... | 0.21 | -0.89 | 0.02 | 0.21 | La II |
Eu II | N/A | ... | ... | -0.3 | -0.82 | 0.09 | -0.3 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Abundances for metal-poor stars with accurate parallaxes I. Basic data
Stellar Parameters
Teff : 5827 | log g : 4.33 | vturb : 0.46 |
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 | ... | 0.53+-0.069 | ... | -0.23+-0.069 | 0.61+-0.069 | 8.46+-0.069 | O I |
Na I | N/A | ... | 0.03+-0.054 | ... | -0.83+-0.054 | 0.01+-0.054 | 5.41+-0.054 | Na I |
Mg I | N/A | ... | 0.45+-0.055 | ... | -0.55+-0.055 | 0.29+-0.055 | 7.05+-0.055 | Mg I |
Si I | N/A | ... | 0.24+-0.048 | ... | -0.57+-0.048 | 0.27+-0.048 | 6.94+-0.048 | Si I |
Ca I | N/A | ... | 0.28+-0.033 | ... | -0.62+-0.033 | 0.22+-0.033 | 5.72+-0.033 | Ca I |
Ti I | N/A | ... | 0.19+-0.03 | ... | -0.52+-0.03 | 0.32+-0.03 | 4.43+-0.03 | Ti I |
Ti II | N/A | ... | 0.25+-0.048 | ... | -0.46+-0.048 | 0.38+-0.048 | 4.49+-0.048 | Ti II |
Fe I | N/A | -0.83+-0.051 | ... | ... | -0.84+-0.051 | ... | 6.66+-0.051 | Fe I |
Fe II | N/A | -0.89+-0.066 | ... | ... | -0.90+-0.066 | ... | 6.60+-0.066 | Fe II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | EMMIESO | 60000 | 150 | N/A | 114.2 |
Cu and Zn in the early Galaxy
Stellar Parameters
Teff : 5823+-70 | log g : 4.29+-0.04 | vturb : 1.0 |
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 | -0.91 | ... | ... | -0.74 | ... | 6.76 | Fe |
Cu I | N/A | -1.16+-0.25 | ... | ... | -1.14+-0.25 | -0.40+-0.25 | 3.05+-0.25 | Cu I |
Zn I | N/A | -0.76+-0.18 | ... | ... | -0.72+-0.18 | 0.02+-0.18 | 3.84+-0.18 | Zn I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ANGLO | 50000 | 80-150 | N/A | N/A |
Oxygen Abundances in Unevolved Metal-poor Stars from Near-Ultraviolet OH Lines
Stellar Parameters
Teff : 5915+-100 | log g : 4.10+-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 |
OH | N/A | -0.38+-0.23 | 0.42 | ... | -0.14+-0.23 | 0.49 | 8.55+-0.23 | OH |
Fe | N/A | -0.80+-0.20 | ... | ... | -0.63+-0.20 | ... | 6.87+-0.20 | Fe |
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 |
N/A | N/A | WHTUES | 50000 | 30-50 | N/A | N/A |
Beryllium abundances and star formation in the halo and in the thick disk
Stellar Parameters
Teff : 5800 | log g : 4.29 | vturb : 1.1 |
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 | ... | ... | 1.45 | -1.81 | -1.01 | 1.45 | Li |
Be | N/A | ... | ... | 0.8 | -0.58 | 0.22 | 0.8 | Be |
Fe | N/A | -0.8 | ... | ... | -0.80 | ... | 6.70 | Fe |
Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
Stellar Parameters
Teff : 5775 | log g : 4.26+-0.07 | vturb : 1.1 |
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 | 5 | ... | 0.04 | ... | -0.70 | 0.12 | 5.54 | Na I |
Mg I | 6 | ... | 0.23 | ... | -0.62 | 0.20 | 6.98 | Mg I |
Al I | 6 | ... | 0.16 | ... | -0.65 | 0.17 | 5.80 | Al I |
Fe | N/A | -0.83 | ... | ... | -0.82 | ... | 6.68 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | 200 | 780 | N/A |
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
Teff : 5792+-100 | log g : 4.29+-0.25 | vturb : 1.2+-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 | -0.95+-0.15 | ... | ... | -0.95+-0.15 | ... | 6.55+-0.15 | Fe |
Sr | N/A | ... | 0.33+-0.14 | ... | -0.62+-0.14 | 0.33+-0.14 | 2.25+-0.14 | Sr |
Y | N/A | ... | -0.06+-0.12 | ... | -1.01+-0.12 | -0.06+-0.12 | 1.20+-0.12 | Y |
Zr | N/A | ... | 0.19+-0.17 | ... | -0.76+-0.17 | 0.19+-0.17 | 1.82+-0.17 | Zr |
Pd | N/A | ... | 0.17+-0.21 | ... | -0.78+-0.21 | 0.17+-0.21 | 0.79+-0.21 | Pd |
Ag | N/A | ... | 0.00+-0.26 | ... | -1.21+-0.26 | -0.26+-0.26 | -0.01+-0.26 | Ag |
Ba | N/A | ... | -0.18+-0.18 | ... | -1.13+-0.18 | -0.18+-0.18 | 1.05+-0.18 | Ba |
Eu | N/A | ... | 0.45+-0.2 | ... | -0.50+-0.2 | 0.45+-0.2 | 0.02+-0.2 | Eu |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 40000 | >100 | N/A | N/A |
Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
Stellar Parameters
Teff : 5759 | log g : 4.25 | 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 |
Fe | N/A | -0.85 | ... | ... | -0.85 | ... | 6.65 | Fe |
Cu | N/A | ... | -0.20+-0.03 | ... | -1.03+-0.03 | -0.18+-0.03 | 3.16+-0.03 | Cu |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 55000 | 250-500 | N/A | N/A |
Observing the metal-poor solar neighbourhood: a comparison of galactic chemical evolution predictions
Stellar Parameters
Teff : 5825+-100 | log g : 4.42+-0.2 | vturb : 0.9+-0.1 |
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 I | N/A | ... | ... | 1.50 | -1.76 | -0.85 | 1.50 | Li I |
O I | N/A | ... | 0.71+-0.20 | ... | -0.18+-0.20 | 0.73+-0.20 | 8.51+-0.20 | O I |
Na I | N/A | ... | -0.02+-0.12 | ... | -0.92+-0.12 | -0.01+-0.12 | 5.32+-0.12 | Na I |
Mg I | N/A | ... | 0.32+-0.10 | ... | -0.65+-0.10 | 0.26+-0.10 | 6.95+-0.10 | Mg I |
Al I | N/A | ... | 0.29+-0.15 | ... | -0.64+-0.15 | 0.27+-0.15 | 5.81+-0.15 | Al I |
Si I | N/A | ... | 0.30+-0.11 | ... | -0.60+-0.11 | 0.31+-0.11 | 6.91+-0.11 | Si I |
Ca I | N/A | ... | 0.26+-0.10 | ... | -0.68+-0.10 | 0.23+-0.10 | 5.66+-0.10 | Ca I |
Sc II | N/A | ... | 0.27+-0.02 | ... | -0.73+-0.02 | 0.18+-0.02 | 2.42+-0.02 | Sc II |
Ti | N/A | ... | 0.30+-0.06 | ... | -0.59+-0.06 | 0.32+-0.06 | 4.36+-0.06 | Ti |
V I | N/A | ... | 0.14+-0.14 | ... | -0.74+-0.14 | 0.17+-0.14 | 3.19+-0.14 | V I |
Cr | N/A | ... | -0.06+-0.08 | ... | -0.96+-0.08 | -0.05+-0.08 | 4.68+-0.08 | Cr |
Mn I | N/A | ... | -0.25+-0.03 | ... | -1.37+-0.03 | -0.46+-0.03 | 4.06+-0.03 | Mn I |
Fe | N/A | -0.91+-0.07 | ... | ... | -0.91+-0.07 | ... | 6.59+-0.07 | Fe |
Co I | N/A | ... | 0.22+-0.11 | ... | -0.72+-0.11 | 0.19+-0.11 | 4.27+-0.11 | Co I |
Ni I | N/A | ... | 0.07+-0.10 | ... | -0.86+-0.10 | 0.05+-0.10 | 5.36+-0.10 | Ni I |
Cu I | N/A | ... | -0.04+-0.04 | ... | -1.08+-0.04 | -0.17+-0.04 | 3.11+-0.04 | Cu I |
Zn I | N/A | ... | 0.16+-0.04 | ... | -0.77+-0.04 | 0.14+-0.04 | 3.79+-0.04 | Zn I |
Sr II | N/A | ... | 0.03+-0.18 | ... | -0.83+-0.18 | 0.08+-0.18 | 2.04+-0.18 | Sr II |
Y II | N/A | ... | 0.12+-0.05 | ... | -0.93+-0.05 | -0.02+-0.05 | 1.28+-0.05 | Y II |
Zr II | N/A | ... | 0.35+-0.02 | ... | -0.54+-0.02 | 0.37+-0.02 | 2.04+-0.02 | Zr II |
Ba II | N/A | ... | 0.09+-0.10 | ... | -0.83+-0.10 | 0.08+-0.10 | 1.35+-0.10 | Ba II |
La II | N/A | ... | 0.3+-0.07 | ... | -0.61+-0.07 | 0.30+-0.07 | 0.49+-0.07 | La II |
Pr II | N/A | ... | 0.3 | ... | -0.52 | 0.39 | 0.20 | Pr II |
Nd II | N/A | ... | 0.12+-0.05 | ... | -0.75+-0.05 | 0.16+-0.05 | 0.67+-0.05 | Nd II |
Eu II | N/A | ... | 0.43 | ... | -0.58 | 0.33 | -0.06 | Eu II |
Position
Right Ascension : 03 40 22.0654223510 | Declination : -03 13 01.124769689 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2013-12-06 | N/A | N/A | 75000 | 207 | N/A | 120.397 |
Elemental abundance survey of the Galactic thick disc
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 |
C | N/A | ... | 0.32 | ... | -0.47 | 0.45 | 7.96 | C |
O | N/A | ... | 0.72 | ... | -0.11 | 0.81 | 8.58 | O |
Na | N/A | ... | 0.1 | ... | -0.74 | 0.18 | 5.50 | Na |
Mg | N/A | ... | 0.44 | ... | -0.49 | 0.43 | 7.11 | Mg |
Al | N/A | ... | 0.22 | ... | -0.82 | 0.10 | 5.63 | Al |
Si | N/A | ... | 0.24 | ... | -0.52 | 0.40 | 6.99 | Si |
Ca | N/A | ... | 0.21 | ... | -0.67 | 0.25 | 5.67 | Ca |
Sc | N/A | ... | 0.16 | ... | -0.62 | 0.30 | 2.53 | Sc |
Ti | N/A | ... | 0.21 | ... | -0.71 | 0.21 | 4.24 | Ti |
V | N/A | ... | 0.19 | ... | -0.61 | 0.31 | 3.32 | V |
Cr | N/A | ... | -0.03 | ... | -0.86 | 0.06 | 4.78 | Cr |
Mn | N/A | ... | -0.39 | ... | -1.32 | -0.40 | 4.11 | Mn |
Fe I | N/A | -0.87 | ... | ... | -0.92 | ... | 6.58 | Fe I |
Co | N/A | ... | 0.11 | ... | -0.82 | 0.10 | 4.17 | Co |
Ni | N/A | ... | -0.02 | ... | -0.88 | 0.04 | 5.34 | Ni |
Cu | N/A | ... | -0.08 | ... | -0.95 | -0.03 | 3.24 | Cu |
Zn | N/A | ... | 0.15 | ... | -0.81 | 0.11 | 3.75 | Zn |
Y | N/A | ... | 0.22 | ... | -0.74 | 0.18 | 1.47 | Y |
Ce | N/A | ... | 0.13 | ... | -0.74 | 0.18 | 0.84 | Ce |
Nd | N/A | ... | 0.25 | ... | -0.54 | 0.38 | 0.88 | Nd |
Eu | N/A | ... | 0.42 | ... | -0.36 | 0.56 | 0.16 | Eu |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-06 | N/A | MCDONALD | 60000 | 100-200 | N/A | 121 |
Abundances of neutron-capture elements in stars of the Galactic disk substructures
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 |
[O I] | N/A | ... | 0.48 | ... | -0.11 | 0.66 | 8.58 | [O I] |
Mg | N/A | ... | 0.42 | ... | -0.37 | 0.40 | 7.23 | Mg |
Si | N/A | ... | 0.28 | ... | -0.45 | 0.32 | 7.06 | Si |
Ca | N/A | ... | 0.25 | ... | -0.50 | 0.27 | 5.84 | Ca |
Fe | N/A | -0.77 | ... | ... | -0.77 | ... | 6.73 | Fe |
Ni | N/A | ... | 0.02 | ... | -0.72 | 0.05 | 5.50 | Ni |
Y | N/A | ... | 0.04 | ... | -0.70 | 0.07 | 1.51 | Y |
Zr | N/A | ... | 0.25 | ... | -0.50 | 0.27 | 2.08 | Zr |
La | N/A | ... | 0.03 | ... | -0.62 | 0.15 | 0.48 | La |
Ce | N/A | ... | -0.01 | ... | -0.81 | -0.04 | 0.77 | Ce |
Nd | N/A | ... | 0.22 | ... | -0.47 | 0.30 | 0.95 | Nd |
Sm | N/A | ... | 0.14 | ... | -0.58 | 0.19 | 0.38 | Sm |
Eu | N/A | ... | 0.41 | ... | -0.37 | 0.40 | 0.15 | Eu |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | ELODIE | 42000 | 100-350 | N/A | N/A |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5759 | log g : 4.25 | 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 |
Na | N/A | ... | 0.1 | ... | -0.66 | 0.19 | 5.58 | Na |
Mg | N/A | ... | 0.36 | ... | -0.51 | 0.34 | 7.09 | Mg |
Si | N/A | ... | 0.32 | ... | -0.49 | 0.36 | 7.02 | Si |
Ca | N/A | ... | 0.3 | ... | -0.53 | 0.32 | 5.81 | Ca |
Ti | N/A | ... | 0.25 | ... | -0.53 | 0.32 | 4.42 | Ti |
Cr | N/A | ... | 0.00 | ... | -0.82 | 0.03 | 4.82 | Cr |
Fe | N/A | -0.85 | ... | ... | -0.85 | ... | 6.65 | Fe |
Ni | N/A | ... | 0.00 | ... | -0.82 | 0.03 | 5.40 | Ni |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-11-26-0327 | N/A | VLT | 55000 | 450 | N/A | 121 |
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 | ... | -0.27 | ... | -1.16 | -0.31 | 4.27 | Mn |
Fe | N/A | -0.85 | ... | ... | -0.85 | ... | 6.65 | Fe |
Cu | N/A | ... | -0.14 | ... | -0.97 | -0.12 | 3.22 | Cu |
Zn | N/A | ... | 0.14 | ... | -0.67 | 0.18 | 3.89 | Zn |
Y | N/A | ... | 0.01 | ... | -0.81 | 0.04 | 1.40 | Y |
Ba | N/A | ... | -0.12 | ... | -1.02 | -0.17 | 1.16 | Ba |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-11-26-0327 | N/A | VLT | 55000 | 450 | N/A | 121 |
Enrichment of the Galactic disc with neutron capture elements: Sr
Stellar Parameters
Teff : 5972 | log g : 4.5 | vturb : 1.1 |
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 | -0.77 | ... | ... | -0.77 | ... | 6.73 | Fe |
Sr | N/A | ... | 0.03 | ... | -0.87 | -0.10 | 2.00 | Sr |
Eu | N/A | ... | 0.41 | ... | -0.37 | 0.40 | 0.15 | Eu |
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 |
| N/A | ELODIE | 42000 | >100 | N/A | N/A |