HD163810
Original Names
BD-13_4807 in C.Charbonnel+,AAP, 442, 961, 2005HIP88010 in T.Bensby+,AAP, 562, A71, 2014
taken from 10 paper(s):
/J.P.Fulbright(2000)/
/D.K.Lai et al.(2007)/
/R.G.Gratton et al.(2003)/
/R.Smiljanic et al.(2009)/
/C.Charbonnel and F. Primas(2005)/
/J.Melendez et al.(2010)/
/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 : 5200 | log g : 4 | vturb : 0.7 |
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 | ... | ... | 1.38 | -1.88 | -0.41 | 1.38 | Li I |
Na I | N/A | ... | -0.21 | ... | -1.61 | -0.14 | 4.63 | Na I |
Mg I | N/A | ... | 0.4 | ... | -1.11 | 0.36 | 6.49 | Mg I |
Al I | N/A | ... | 0.17 | ... | -1.30 | 0.17 | 5.15 | Al I |
Si I | N/A | ... | 0.25 | ... | -1.20 | 0.27 | 6.31 | Si I |
Ca I | N/A | ... | 0.36 | ... | -1.11 | 0.36 | 5.23 | Ca I |
Ti | N/A | ... | 0.18 | ... | -1.27 | 0.20 | 3.68 | Ti |
V I | N/A | ... | -0.01 | ... | -1.43 | 0.04 | 2.50 | V I |
Cr I | N/A | ... | 0.06 | ... | -1.40 | 0.07 | 4.24 | Cr I |
Fe | N/A | -1.49 | ... | ... | -1.47 | ... | 6.03 | Fe |
Ni I | N/A | ... | -0.03 | ... | -1.49 | -0.02 | 4.73 | Ni I |
Y II | N/A | ... | -0.23 | ... | -1.69 | -0.22 | 0.52 | Y II |
Zr II | N/A | ... | 0.24 | ... | -1.23 | 0.24 | 1.35 | Zr II |
Ba II | N/A | ... | -0.01 | ... | -1.55 | -0.08 | 0.63 | Ba II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998-08-08 | N/A | LICKHAMILTON | 50000 | 95 | 2700 | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
D.K.Lai et al.,ApJ, 667, 1185, 2007 (A0128,ADS)
Carbon and Strontium Abundances of Metal-poor 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 |
C | N/A | ... | -0.50+-0.17 | ... | -1.68+-0.17 | -0.54+-0.17 | 6.75+-0.17 | C |
Fe | N/A | -1.31 | ... | ... | -1.14 | ... | 6.36 | Fe |
Sr | N/A | ... | 0.11 | ... | -1.17 | -0.03 | 1.70 | Sr |
Ba | N/A | ... | 0.09 | ... | -1.27 | -0.13 | 0.91 | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKII | 7000 | N/A | 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 : 5422 | log g : 4.23 | vturb : 0.9 |
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 | ... | -0.18+-0.054 | ... | -1.57+-0.054 | -0.20+-0.054 | 4.67+-0.054 | Na I |
Mg I | N/A | ... | 0.41+-0.055 | ... | -1.12+-0.055 | 0.25+-0.055 | 6.48+-0.055 | Mg I |
Si I | N/A | ... | 0.17+-0.048 | ... | -1.17+-0.048 | 0.20+-0.048 | 6.34+-0.048 | Si I |
Ca I | N/A | ... | 0.36+-0.033 | ... | -1.07+-0.033 | 0.30+-0.033 | 5.27+-0.033 | Ca I |
Ti I | N/A | ... | 0.17+-0.03 | ... | -1.07+-0.03 | 0.30+-0.03 | 3.88+-0.03 | Ti I |
Ti II | N/A | ... | 0.08+-0.048 | ... | -1.16+-0.048 | 0.21+-0.048 | 3.79+-0.048 | Ti II |
Fe I | N/A | -1.36+-0.051 | ... | ... | -1.37+-0.051 | ... | 6.13+-0.051 | Fe I |
Fe II | N/A | -1.44+-0.066 | ... | ... | -1.45+-0.066 | ... | 6.05+-0.066 | Fe II |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | N/A | 50000 | >100 | N/A | 191 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -130550 | Right Ascension : 175838 |
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 : 5200 | log g : 4.15 | vturb : 0.7 |
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 | ... | ... | 1.67 | -1.59 | -0.19 | 1.67 | Li |
Be | N/A | ... | ... | -0.34 | -1.72 | -0.32 | -0.34 | Be |
Fe | N/A | -1.4 | ... | ... | -1.40 | ... | 6.10 | Fe |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
C.Charbonnel et al.,AAP, 442, 961, 2005 (A0191,ADS)
The lithium content of the Galactic Halo 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 |
Li I | N/A | ... | ... | 1.599+0.041-0.046 | ... | ... | Li I |
Fe | N/A | -1.36+-0.120 | ... | ... | ... | ... | Fe |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -13.09712 | Right Ascension : 269.66022 |
J.Melendez et al.,AAP, 515, L3, 2010 (A0235,ADS)
Observational evidence for a broken Li Spite plateau and mass-dependent Li depletion
Stellar Parameters
Teff : 5602+-50 | log g : 4.59 |
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 | ... | ... | 1.64+-0.035 | -1.62+-0.035 | -0.33+-0.035 | 1.64+-0.035 | Li |
Fe | N/A | -1.29 | ... | ... | -1.29 | ... | 6.21 | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | VLT | 110000 | >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, 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 : 5424+-77 | log g : 4.43+-0.10 | vturb : 1.01+-0.27 |
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 | ... | 0.77+-0.21 | ... | ... | ... | O |
Na | 2 | ... | -0.22+-0.04 | ... | ... | ... | Na |
Mg | 2 | ... | 0.34+-0.08 | ... | ... | ... | Mg |
Si | 18 | ... | 0.14+-0.10 | ... | ... | ... | Si |
Ca | 15 | ... | 0.30+-0.08 | ... | ... | ... | Ca |
Ti | 19 | -1.12+-0.10 | 0.22+-0.10 | ... | ... | Ti |
Cr | 6 | ... | 0.06+-0.07 | ... | ... | ... | Cr |
Fe | 161 | -1.34+-0.08 | ... | ... | ... | ... | Fe |
Fe I | 147 | ... | ... | 6.25 | ... | ... | Fe I |
Fe II | 14 | ... | ... | 6.25 | ... | ... | Fe II |
Ni | 23 | ... | -0.15+-0.09 | ... | ... | ... | Ni |
Zn | 2 | ... | 0.05+-0.16 | ... | ... | ... | Zn |
Y | 3 | ... | -0.10+-0.21 | ... | ... | ... | Y |
Ba | 3 | ... | -0.09+-0.16 | ... | ... | ... | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-04-01 | N/A | MIKELCO | 65000 | 250 | 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 | ... | -0.21 | ... | ... | ... | Na |
Mg | N/A | ... | 0.4 | ... | ... | ... | Mg |
Ca | N/A | ... | 0.36 | ... | ... | ... | Ca |
Ti | N/A | ... | 0.18 | ... | ... | ... | Ti |
Fe | N/A | -1.49 | ... | ... | ... | ... | Fe |
Ni | N/A | ... | -0.03 | ... | ... | ... | Ni |
Y | N/A | ... | -0.23 | ... | ... | ... | Y |
Ba | N/A | ... | -0.01 | ... | ... | ... | Ba |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -130550 | Right Ascension : 175838.5 |
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 : 5501 | log g : 4.56 | 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 | ... | -0.22 | ... | -1.33 | -0.13 | 4.91 | Na |
Mg | N/A | ... | 0.18 | ... | -1.04 | 0.16 | 6.56 | Mg |
Si | N/A | ... | 0.17 | ... | -0.99 | 0.21 | 6.52 | Si |
Ca | N/A | ... | 0.28 | ... | -0.90 | 0.30 | 5.44 | Ca |
Ti | N/A | ... | 0.22 | ... | -0.91 | 0.29 | 4.04 | Ti |
Cr | N/A | ... | 0.02 | ... | -1.15 | 0.05 | 4.49 | Cr |
Fe | N/A | -1.20 | ... | ... | -1.20 | ... | 6.30 | Fe |
Ni | N/A | ... | -0.1 | ... | -1.27 | -0.07 | 4.95 | Ni |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-04-27-0823 | N/A | VLT | 55000 | 300 | N/A | 185.9 |
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 | ... | -0.30 | ... | -1.54 | -0.34 | 3.89 | Mn |
Fe | N/A | -1.2 | ... | ... | -1.20 | ... | 6.30 | Fe |
Cu | N/A | ... | -0.55 | ... | -1.73 | -0.53 | 2.46 | Cu |
Zn | N/A | ... | 0.02 | ... | -1.14 | 0.06 | 3.42 | Zn |
Y | N/A | ... | -0.11 | ... | -1.28 | -0.08 | 0.93 | Y |
Ba | N/A | ... | -0.16 | ... | -1.41 | -0.21 | 0.77 | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-04-27-0823 | N/A | VLT | 55000 | 300 | N/A | 185.9 |