HD163810
Original Names
BD-13_4807 in C.Charbonnel+,AAP, 442, 961, 2005HIP88010 in T.Bensby+,AAP, 562, A71, 2014
taken from 8 paper(s):
/J.P.Fulbright(2000)/
/D.K.Lai et al.(2007)/
/R.G.Gratton et al.(2003)/
/R.Smiljanic et al.(2009)/
/J.Melendez et al.(2010)/
/H.L.Yan et al.(2016)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
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 |
Position
Right Ascension : 17 58 38.45 | Declination : -13 05 49.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998-08-08 | N/A | LICKHAMILTON | 50000 | 95 | 2700 | N/A |
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 |
Position
Right Ascension : 17 58 38.45 | Declination : -13 05 49.6 | 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 | KECKII | 7000 | N/A | N/A | N/A |
Abundances for metal-poor stars with accurate parallaxes I. Basic data
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
Position
Right Ascension : 17 58 38.45 | Declination : -13 05 49.6 | 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 | 50000 | >100 | N/A | 191 |
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 |
Position
Right Ascension : 17 58 38.45 | Declination : -13 05 49.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
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 |
Position
Right Ascension : 17 58 38.45 | Declination : -13 05 49.6 | 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 | VLT | 110000 | >100 | N/A | N/A |
Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
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 |
Fe | N/A | -1.2 | ... | ... | -1.20 | ... | 6.30 | Fe |
Cu | N/A | ... | -0.54+-0.03 | ... | -1.72+-0.03 | -0.52+-0.03 | 2.47+-0.03 | Cu |
Position
Right Ascension : 17 58 38.45 | Declination : -13 05 49.6 | 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 | VLT | 55000 | 250-500 | N/A | N/A |
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 |
Position
Right Ascension : 17 58 38.45 | Declination : -13 05 49.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
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 |
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 |
Position
Right Ascension : 17 58 38.45 | Declination : -13 05 49.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
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 |