HD022879
Original Names
BD-03_592 in E.Caffau+,AAP, 441, 533, 2005HD22879 in J.P.Fulbright+,AJ, 120, 1841, 2000HIP17147 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)/
/E.Caffau et al.(2005)/
/R.Smiljanic et al.(2009)/
/T.Gehren et al.(2006)/
/C.J.Hansen et al.(2012)/
/T.Bensby et al.(2005)/
/B.E.Reddy et al.(2006)/
/T.V.Mishenina et al.(2013)/
/T.Bensby et al.(2014)/
/K.A.Venn et al.(2004)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/

J.P.Fulbright et al.,AJ, 120, 1841, 2000 (A0126,ADS)
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 | ... | ... | Li I |
Na I | N/A | ... | 0.08 | ... | ... | ... | Na I |
Mg I | N/A | ... | 0.41 | ... | ... | ... | Mg I |
Al I | N/A | ... | 0.31 | ... | ... | ... | Al I |
Si I | N/A | ... | 0.35 | ... | ... | ... | Si I |
Ca I | N/A | ... | 0.26 | ... | ... | ... | Ca I |
Ti | N/A | ... | 0.32 | ... | ... | ... | Ti |
V I | N/A | ... | 0.18 | ... | ... | ... | V I |
Cr I | N/A | ... | 0.03 | ... | ... | ... | Cr I |
Fe | N/A | -0.91 | ... | ... | ... | ... | Fe |
Ni I | N/A | ... | 0.02 | ... | ... | ... | Ni I |
Y II | N/A | ... | 0.05 | ... | ... | ... | Y II |
Zr II | N/A | ... | 0.27 | ... | ... | ... | Zr II |
Ba II | N/A | ... | 0.11 | ... | ... | ... | Ba II |
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 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
J.Simmerer et al.,ApJ, 617, 1091, 2004 (A0131,ADS)
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 | ... | ... | ... | ... | Fe I |
Fe II | N/A | -1.03 | ... | ... | ... | ... | Fe II |
La II | N/A | ... | ... | 0.21 | ... | ... | La II |
Eu II | N/A | ... | ... | -0.3 | ... | ... | Eu II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
R.G.Gratton et al.,AAP, 404, 187, 2003 (A0135,ADS)
Abundances for metal-poor stars with accurate parallaxes
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 | ... | ... | ... | O I |
Na I | N/A | ... | 0.03+-0.054 | ... | ... | ... | Na I |
Mg I | N/A | ... | 0.45+-0.055 | ... | ... | ... | Mg I |
Si I | N/A | ... | 0.24+-0.048 | ... | ... | ... | Si I |
Ca I | N/A | ... | 0.28+-0.033 | ... | ... | ... | Ca I |
Ti I | N/A | ... | 0.19+-0.03 | ... | ... | ... | Ti I |
Ti II | N/A | ... | 0.25+-0.048 | ... | ... | ... | Ti II |
Fe I | N/A | -0.83+-0.051 | ... | ... | ... | ... | Fe I |
Fe II | N/A | -0.89+-0.066 | ... | ... | ... | ... | Fe II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | EMMIESO | 60000 | 150 | N/A | 114.2 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -31301 | Right Ascension : 34022 |
G.Bihain et al.,AAP, 423, 777, 2004 (A0136,ADS)
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 | ... | ... | ... | ... | Fe |
Cu I | N/A | -1.16+-0.25 | ... | ... | ... | ... | Cu I |
Zn I | N/A | -0.76+-0.18 | ... | ... | ... | ... | Zn I |
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 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
E.Caffau et al.,AAP, 441, 533, 2005 (A0137,ADS)
Sulphur abundance in Galactic stars
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 |
S I | N/A | -0.69+-0.11 | 0.14+-0.11 | ... | ... | S I |
Fe | N/A | -0.83 | ... | ... | ... | ... | Fe |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | 2450086.56539 | EMMIESO | 60000 | 300 | N/A | |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -31301 | Right Ascension : 34022 |
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 : 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 | ... | ... | Li |
Be | N/A | ... | ... | 0.8 | ... | ... | Be |
Fe | N/A | -0.8 | ... | ... | ... | ... | Fe |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
T.Gehren et al.,AAP, 451, 1065, 2006 (A0259,ADS)
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 | ... | ... | ... | Na I |
Mg I | 6 | ... | 0.23 | ... | ... | ... | Mg I |
Al I | 6 | ... | 0.16 | ... | ... | ... | Al I |
Fe | N/A | -0.83 | ... | ... | ... | ... | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | 200 | 780 | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -031259.3 | Right Ascension : 034021.66 |
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 : 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 | ... | ... | ... | ... | Fe |
Sr | N/A | ... | 0.33+-0.14 | ... | ... | ... | Sr |
Y | N/A | ... | -0.06+-0.12 | ... | ... | ... | Y |
Zr | N/A | ... | 0.19+-0.17 | ... | ... | ... | Zr |
Pd | N/A | ... | 0.17+-0.21 | ... | ... | ... | Pd |
Ag | N/A | ... | 0.00+-0.26 | ... | ... | ... | Ag |
Ba | N/A | ... | -0.18+-0.18 | ... | ... | ... | Ba |
Eu | N/A | ... | 0.45+-0.2 | ... | ... | ... | 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 |
T.Bensby et al.,AAP, 433, 185, 2005 (C0001,ADS)
alpha-, r-, and s-process element trends in the Galactic thin and thick disks
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 | 4 | -0.75+-0.04 | ... | ... | ... | ... | Na I |
Mg I | 6 | -0.44+-0.04 | ... | ... | ... | ... | Mg I |
Al I | 4 | -0.50+-0.01 | ... | ... | ... | ... | Al I |
Si I | 29 | -0.57+-0.10 | ... | ... | ... | ... | Si I |
Ca I | 22 | -0.58+-0.12 | ... | ... | ... | ... | Ca I |
Ti I | 25 | -0.53+-0.10 | ... | ... | ... | ... | Ti I |
Ti II | 18 | -0.55+-0.12 | ... | ... | ... | ... | Ti II |
Cr I | 10 | -0.75+-0.13 | ... | ... | ... | ... | Cr I |
Cr II | 7 | -0.92+-0.07 | ... | ... | ... | ... | Cr II |
Fe I | 120 | -0.84+-0.09 | ... | ... | ... | ... | Fe I |
Fe II | 24 | -0.88+-0.12 | ... | ... | ... | ... | Fe II |
Ni I | 42 | -0.83+-0.14 | ... | ... | ... | ... | Ni I |
Zn I | 2 | -0.72+-0.04 | ... | ... | ... | ... | Zn I |
Y II | 6 | -0.88+-0.16 | ... | ... | ... | ... | Y II |
Ba II | 4 | -0.81+-0.06 | ... | ... | ... | ... | Ba II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-09-01 | N/A | FEROSESO | 48000 | 150-250 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
B.E.Reddy et al.,MNRAS, 367, 1329, 2006 (C0002,ADS)
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 | ... | ... | ... | C |
O | N/A | ... | 0.72 | ... | ... | ... | O |
Na | N/A | ... | 0.1 | ... | ... | ... | Na |
Mg | N/A | ... | 0.44 | ... | ... | ... | Mg |
Al | N/A | ... | 0.22 | ... | ... | ... | Al |
Si | N/A | ... | 0.24 | ... | ... | ... | Si |
Ca | N/A | ... | 0.21 | ... | ... | ... | Ca |
Sc | N/A | ... | 0.16 | ... | ... | ... | Sc |
Ti | N/A | ... | 0.21 | ... | ... | ... | Ti |
V | N/A | ... | 0.19 | ... | ... | ... | V |
Cr | N/A | ... | -0.03 | ... | ... | ... | Cr |
Mn | N/A | ... | -0.39 | ... | ... | ... | Mn |
Fe I | N/A | -0.87 | ... | ... | ... | ... | Fe I |
Co | N/A | ... | 0.11 | ... | ... | ... | Co |
Ni | N/A | ... | -0.02 | ... | ... | ... | Ni |
Cu | N/A | ... | -0.08 | ... | ... | ... | Cu |
Zn | N/A | ... | 0.15 | ... | ... | ... | Zn |
Y | N/A | ... | 0.22 | ... | ... | ... | Y |
Ce | N/A | ... | 0.13 | ... | ... | ... | Ce |
Nd | N/A | ... | 0.25 | ... | ... | ... | Nd |
Eu | N/A | ... | 0.42 | ... | ... | ... | Eu |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-06 | N/A | MCDONALD | 60000 | 100-200 | N/A | 121 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
T.V.Mishenina et al.,AAP, 552, A128, 2013 (C0005,ADS)
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 | ... | ... | ... | [O I] |
Mg | N/A | ... | 0.42 | ... | ... | ... | Mg |
Si | N/A | ... | 0.28 | ... | ... | ... | Si |
Ca | N/A | ... | 0.25 | ... | ... | ... | Ca |
Fe | N/A | -0.77 | ... | ... | ... | ... | Fe |
Ni | N/A | ... | 0.02 | ... | ... | ... | Ni |
Y | N/A | ... | 0.04 | ... | ... | ... | Y |
Zr | N/A | ... | 0.25 | ... | ... | ... | Zr |
La | N/A | ... | 0.03 | ... | ... | ... | La |
Ce | N/A | ... | -0.01 | ... | ... | ... | Ce |
Nd | N/A | ... | 0.22 | ... | ... | ... | Nd |
Sm | N/A | ... | 0.14 | ... | ... | ... | Sm |
Eu | N/A | ... | 0.41 | ... | ... | ... | Eu |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | ELODIE | 42000 | 100-350 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -3.21698 | Right Ascension : 55.09193 |
T.Bensby et al.,AAP, 562, A71, 2014 (C0007,ADS)
Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the solar neighbourhood
Stellar Parameters
Teff : 5970+-150 | log g : 4.52+-0.15 | vturb : 1.27+-1.00 |
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 | 3 | ... | 0.53 | ... | ... | ... | O |
Na | 4 | ... | 0.06 | ... | ... | ... | Na |
Mg | 6 | ... | 0.35 | ... | ... | ... | Mg |
Al | 4 | ... | 0.33 | ... | ... | ... | Al |
Si | 29 | ... | 0.23 | ... | ... | ... | Si |
Ca | 22 | ... | 0.24 | ... | ... | ... | Ca |
Ti | 43 | -0.48 | 0.33 | ... | ... | Ti |
Cr | 17 | ... | 0.03 | ... | ... | ... | Cr |
Fe | 150 | -0.81+-0.15 | ... | ... | ... | ... | Fe |
Fe I | 121 | ... | ... | 6.75 | ... | ... | Fe I |
Fe II | 29 | ... | ... | 6.75 | ... | ... | Fe II |
Ni | 43 | ... | 0.01 | ... | ... | ... | Ni |
Zn | 3 | ... | 0.09 | ... | ... | ... | Zn |
Y | 6 | ... | 0.12 | ... | ... | ... | Y |
Ba | 4 | ... | -0.01 | ... | ... | ... | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-01-01 | N/A | FEROSESO | 48000 | 150 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
K.A.Venn et al.,AJ, 128, 1177, 2004 (C0011,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 |
Na | N/A | ... | 0.09 | ... | ... | ... | Na |
Mg | N/A | ... | 0.4 | ... | ... | ... | Mg |
Ca | N/A | ... | 0.26 | ... | ... | ... | Ca |
Ti | N/A | ... | 0.3 | ... | ... | ... | Ti |
Fe | N/A | -0.84 | ... | ... | ... | ... | Fe |
Ni | N/A | ... | 0.01 | ... | ... | ... | Ni |
Y | N/A | ... | 0.05 | ... | ... | ... | Y |
Ba | N/A | ... | 0.11 | ... | ... | ... | Ba |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -031301 | Right Ascension : 034022.1 |
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 : 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 | ... | ... | ... | Na |
Mg | N/A | ... | 0.36 | ... | ... | ... | Mg |
Si | N/A | ... | 0.32 | ... | ... | ... | Si |
Ca | N/A | ... | 0.3 | ... | ... | ... | Ca |
Ti | N/A | ... | 0.25 | ... | ... | ... | Ti |
Cr | N/A | ... | 0.00 | ... | ... | ... | Cr |
Fe | N/A | -0.85 | ... | ... | ... | ... | Fe |
Ni | N/A | ... | 0.00 | ... | ... | ... | Ni |
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 |
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 | ... | -0.27 | ... | ... | ... | Mn |
Fe | N/A | -0.85 | ... | ... | ... | ... | Fe |
Cu | N/A | ... | -0.14 | ... | ... | ... | Cu |
Zn | N/A | ... | 0.14 | ... | ... | ... | Zn |
Y | N/A | ... | 0.01 | ... | ... | ... | Y |
Ba | N/A | ... | -0.12 | ... | ... | ... | Ba |
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 |