HD113679
Original Names
CD-37_8363 in E.Caffau+,AAP, 441, 533, 2005HIP63918 in T.Bensby+,AAP, 562, A71, 2014
taken from 8 paper(s):
/P.E.Nissen et al.(2002)/
/R.G.Gratton et al.(2003)/
/K.F.Tan et al.(2009)/
/R.Smiljanic et al.(2009)/
/C.J.Hansen et al.(2012)/
/H.L.Yan et al.(2016)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
O/Fe in metal-poor main sequence and subgiant stars
Stellar Parameters
| Teff : 5678 | log g : 4.04 | 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 |
|---|
| [O I] | N/A | ... | 0.31+-0.05 | 8.39+-0.05 | -0.30+-0.05 | 0.33+-0.05 | 8.39+-0.05 | [O I] |
| Fe | N/A | -0.66 | ... | ... | -0.63 | ... | 6.87 | Fe |
Position
| Right Ascension : 13 05 52.80 | Declination : -38 31 00.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2000-04 | N/A | VLT | 55000 | 300-400 | N/A | N/A |
Abundances for metal-poor stars with accurate parallaxes I. Basic data
Stellar Parameters
| Teff : 5543 | log g : 3.88 | vturb : 0.6 |
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 | ... | 0.55+-0.069 | ... | -0.08+-0.069 | 0.63+-0.069 | 8.61+-0.069 | O I |
| Na I | N/A | ... | 0.05+-0.054 | ... | -0.68+-0.054 | 0.03+-0.054 | 5.56+-0.054 | Na I |
| Mg I | N/A | ... | 0.41+-0.055 | ... | -0.46+-0.055 | 0.25+-0.055 | 7.14+-0.055 | Mg I |
| Si I | N/A | ... | 0.27+-0.048 | ... | -0.41+-0.048 | 0.30+-0.048 | 7.10+-0.048 | Si I |
| Ca I | N/A | ... | 0.31+-0.033 | ... | -0.46+-0.033 | 0.25+-0.033 | 5.88+-0.033 | Ca I |
| Ti I | N/A | ... | 0.21+-0.03 | ... | -0.37+-0.03 | 0.34+-0.03 | 4.58+-0.03 | Ti I |
| Ti II | N/A | ... | 0.42+-0.048 | ... | -0.16+-0.048 | 0.55+-0.048 | 4.79+-0.048 | Ti II |
| Fe I | N/A | -0.7+-0.051 | ... | ... | -0.71+-0.051 | ... | 6.79+-0.051 | Fe I |
| Fe II | N/A | -0.66+-0.066 | ... | ... | -0.67+-0.066 | ... | 6.83+-0.066 | Fe II |
Binary Parameters
Position
| Right Ascension : 13 05 52.80 | Declination : -38 31 00.0 | 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 | EMMIESO | 60000 | 150 | N/A | 156 |
Beryllium abundances in metal-poor stars
Stellar Parameters
| Teff : 5740+-80 | log g : 3.94+-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 |
|---|
| Li | N/A | ... | ... | 2.05 | -1.21 | -0.52 | 2.05 | Li |
| Be | N/A | ... | ... | 0.87+-0.12 | -0.51+-0.12 | 0.18+-0.12 | 0.87+-0.12 | Be |
| O | N/A | -0.15 | ... | ... | -0.07 | 0.62 | 8.62 | O |
| Ti | N/A | ... | 0.32 | ... | -0.39 | 0.30 | 4.56 | Ti |
| Fe | N/A | -0.70 | ... | ... | -0.69 | ... | 6.81 | Fe |
Position
| Right Ascension : 13 05 52.80 | Declination : -38 31 00.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2008-04-10 | N/A | VLT | 48000 | N/A | N/A | N/A |
Beryllium abundances and star formation in the halo and in the thick disk
Stellar Parameters
| Teff : 5720 | log g : 3.91 | vturb : 1.49 |
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 | ... | ... | 1.99 | -1.27 | -0.62 | 1.99 | Li |
| Be | N/A | ... | ... | 1.05 | -0.33 | 0.32 | 1.05 | Be |
| Fe | N/A | -0.65 | ... | ... | -0.65 | ... | 6.85 | Fe |
Position
| Right Ascension : 13 05 52.80 | Declination : -38 31 00.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
| Teff : 5759+-100 | log g : 4.04+-0.25 | vturb : 0.9+-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 | -0.63+-0.15 | ... | ... | -0.63+-0.15 | ... | 6.87+-0.15 | Fe |
| Sr | N/A | ... | <0.44 | ... | <-0.19 | <0.44 | <2.68 | Sr |
| Y | N/A | ... | 0.08+-0.12 | ... | -0.55+-0.12 | 0.08+-0.12 | 1.66+-0.12 | Y |
| Zr | N/A | ... | 0.22+-0.17 | ... | -0.41+-0.17 | 0.22+-0.17 | 2.17+-0.17 | Zr |
| Pd | N/A | ... | 0.14+-0.19 | ... | -0.49+-0.19 | 0.14+-0.19 | 1.08+-0.19 | Pd |
| Ag | N/A | ... | 0.08+-0.25 | ... | -0.81+-0.25 | -0.18+-0.25 | 0.39+-0.25 | Ag |
| Ba | N/A | ... | 0.25+-0.15 | ... | -0.38+-0.15 | 0.25+-0.15 | 1.80+-0.15 | Ba |
| Eu | N/A | ... | 0.08+-0.21 | ... | -0.55+-0.21 | 0.08+-0.21 | -0.03+-0.21 | Eu |
Position
| Right Ascension : 13 05 52.80 | Declination : -38 31 00.0 | 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 | 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 : 5672 | log g : 3.99 | vturb : 1.4 |
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 |
|---|
| Fe | N/A | -0.65 | ... | ... | -0.65 | ... | 6.85 | Fe |
| Cu | N/A | ... | -0.13+-0.00 | ... | -0.76+-0.00 | -0.11+-0.00 | 3.43+-0.00 | Cu |
Position
| Right Ascension : 13 05 52.80 | Declination : -38 31 00.0 | 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 : 5672 | log g : 3.99 | vturb : 1.4 |
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 | N/A | ... | 0.15 | ... | -0.41 | 0.24 | 5.83 | Na |
| Mg | N/A | ... | 0.37 | ... | -0.30 | 0.35 | 7.30 | Mg |
| Si | N/A | ... | 0.33 | ... | -0.28 | 0.37 | 7.23 | Si |
| Ca | N/A | ... | 0.32 | ... | -0.31 | 0.34 | 6.03 | Ca |
| Ti | N/A | ... | 0.26 | ... | -0.32 | 0.33 | 4.63 | Ti |
| Cr | N/A | ... | 0.02 | ... | -0.60 | 0.05 | 5.04 | Cr |
| Fe | N/A | -0.65 | ... | ... | -0.65 | ... | 6.85 | Fe |
| Ni | N/A | ... | 0.03 | ... | -0.59 | 0.06 | 5.63 | Ni |
Position
| Right Ascension : 13 05 52.80 | Declination : -38 31 00.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2000-04-10-0439 | N/A | VLT | 55000 | 500 | N/A | 158 |
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 | ... | -0.23 | ... | -0.92 | -0.27 | 4.51 | Mn |
| Fe | N/A | -0.65 | ... | ... | -0.65 | ... | 6.85 | Fe |
| Cu | N/A | ... | -0.07 | ... | -0.70 | -0.05 | 3.49 | Cu |
| Zn | N/A | ... | 0.17 | ... | -0.44 | 0.21 | 4.12 | Zn |
| Y | N/A | ... | -0.01 | ... | -0.63 | 0.02 | 1.58 | Y |
| Ba | N/A | ... | -0.17 | ... | -0.87 | -0.22 | 1.31 | Ba |
Position
| Right Ascension : 13 05 52.80 | Declination : -38 31 00.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2000-04-10-0439 | N/A | VLT | 55000 | 500 | N/A | 158 |