HD199289
taken from 7 paper(s):
/R.G.Gratton et al.(2000)/
/K.Jonsell et al.(2005)/
/R.Smiljanic et al.(2009)/
/J.Melendez et al.(2010)/
/K.A.Venn et al.(2004)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/

R.G.Gratton et al.,AAP, 354, 169, 2000 (A0049,ADS)
Mixing along the red giant branch in metal-poor field stars
Stellar Parameters
Teff : 5890 | log g : 4.05 | vturb : 1.10 |
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 | ... | ... | 2.00 | -1.26 | -0.19 | 2.00 | Li I |
C | N/A | ... | -0.04 | ... | -0.99 | 0.08 | 7.44 | C |
O | N/A | ... | 0.21 | ... | -0.63 | 0.44 | 8.06 | O |
Na | N/A | ... | 0.12 | ... | -0.91 | 0.16 | 5.33 | Na |
Fe I | N/A | -1.02 | ... | ... | -1.07 | ... | 6.43 | Fe I |
Isotopic Ratio
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1995-05 | N/A | CESESO | 50000 | 80-150 | N/A | N/A |
1995-11 | N/A | CESESO | 50000 | 80-150 | N/A | N/A |
1995-11 | N/A | MCDONALD | 60000 | 70-100 | N/A | N/A |
Galactic Longitude (l) : 351.31 | Galactic Latitude (b) : -40.65 | Declination : -481213 | Right Ascension : 205808.5 |
K.Jonsell et al.,AAP, 440, 321, 2005 (A0078,ADS)
Chemical abundances in 43 metal-poor stars
Stellar Parameters
Teff : 5800 | log g : 4.21 | vturb : 1.5 |
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 | ... | 0.60 | ... | -0.53 | 0.57 | 8.16 | O I |
Na I | N/A | ... | 0.13 | ... | -0.88 | 0.22 | 5.36 | Na I |
Mg I | N/A | ... | 0.32 | ... | -0.80 | 0.30 | 6.80 | Mg I |
Al I | N/A | ... | 0.29 | ... | -0.79 | 0.31 | 5.66 | Al I |
Si I | N/A | ... | 0.27 | ... | -0.79 | 0.31 | 6.72 | Si I |
Ca I | N/A | ... | 0.22 | ... | -0.86 | 0.24 | 5.48 | Ca I |
Ti I | N/A | ... | 0.29 | ... | -0.74 | 0.36 | 4.21 | Ti I |
V I | N/A | ... | 0.16 | ... | -0.87 | 0.23 | 3.06 | V I |
Cr I | N/A | ... | -0.09 | ... | -1.16 | -0.06 | 4.48 | Cr I |
Fe | N/A | -1.10 | ... | ... | -1.10 | ... | 6.40 | Fe |
Fe II | N/A | ... | 0.05 | ... | -1.05 | 0.05 | 6.45 | Fe II |
Ni I | N/A | ... | 0.03 | ... | -1.04 | 0.06 | 5.18 | Ni I |
Ba II | N/A | ... | -0.28 | ... | -1.43 | -0.33 | 0.75 | Ba II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | CATCESESO | 60000 | 200 | N/A | N/A |
Galactic Longitude (l) : 351.313 | Galactic Latitude (b) : -40.649 | Declination : -48.2037 | Right Ascension : 314.5355 |
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 : 5894 | log g : 4.29 | vturb : 1.32 |
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 | -1.26 | -0.23 | 2 | Li |
Be | N/A | ... | ... | 0.61 | -0.77 | 0.26 | 0.61 | Be |
Fe | N/A | -1.03 | ... | ... | -1.03 | ... | 6.47 | Fe |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
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 : 5975+-50 | log g : 4.35 |
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 | ... | ... | 1.93+-0.035 | -1.33+-0.035 | -0.31+-0.035 | 1.93+-0.035 | Li |
Fe | N/A | -1.02 | ... | ... | -1.02 | ... | 6.48 | 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 |
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 | ... | 0.1 | ... | -0.84 | 0.19 | 5.40 | Na |
Mg | N/A | ... | 0.4 | ... | -0.65 | 0.38 | 6.95 | Mg |
Ca | N/A | ... | 0.23 | ... | -0.78 | 0.25 | 5.56 | Ca |
Ti | N/A | ... | 0.28 | ... | -0.68 | 0.35 | 4.27 | Ti |
Fe | N/A | -1.03 | ... | ... | -1.03 | ... | 6.47 | Fe |
Ni | N/A | ... | 0.05 | ... | -0.95 | 0.08 | 5.27 | Ni |
Y | N/A | ... | 0.01 | ... | -0.99 | 0.04 | 1.22 | Y |
Ba | N/A | ... | -0.25 | ... | -1.33 | -0.30 | 0.85 | Ba |
Eu | N/A | ... | 0.26 | ... | -0.78 | 0.25 | -0.26 | Eu |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -481213 | Right Ascension : 205808.5 |
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 : 5810 | log g : 4.28 | 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 | ... | 0.08 | ... | -0.87 | 0.17 | 5.37 | Na |
Mg | N/A | ... | 0.36 | ... | -0.70 | 0.34 | 6.90 | Mg |
Si | N/A | ... | 0.31 | ... | -0.69 | 0.35 | 6.82 | Si |
Ca | N/A | ... | 0.27 | ... | -0.75 | 0.29 | 5.59 | Ca |
Ti | N/A | ... | 0.24 | ... | -0.73 | 0.31 | 4.22 | Ti |
Cr | N/A | ... | -0.02 | ... | -1.03 | 0.01 | 4.61 | Cr |
Fe | N/A | -1.04 | ... | ... | -1.04 | ... | 6.46 | Fe |
Ni | N/A | ... | 0.02 | ... | -0.99 | 0.05 | 5.23 | Ni |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-06-04-0125 | N/A | VLT | 55000 | 290 | N/A | -5.6 |
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 | ... | -0.26 | ... | -1.34 | -0.30 | 4.09 | Mn |
Fe | N/A | -1.04 | ... | ... | -1.04 | ... | 6.46 | Fe |
Cu | N/A | ... | -0.17 | ... | -1.19 | -0.15 | 3.00 | Cu |
Zn | N/A | ... | 0.13 | ... | -0.87 | 0.17 | 3.69 | Zn |
Y | N/A | ... | -0.09 | ... | -1.10 | -0.06 | 1.11 | Y |
Ba | N/A | ... | -0.21 | ... | -1.30 | -0.26 | 0.88 | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-06-04-0125 | N/A | VLT | 55000 | 290 | N/A | -5.6 |