HD149414
Original Names
G17-25 in J.Simmerer+,ApJ, 617, 1091, 2004HIP81170 in K.A.Venn+,AJ, 128, 1177, 2004
taken from 11 paper(s):
/G.S.Bai et al.(2004)/
/J.P.Fulbright(2000)/
/J.Simmerer et al.(2004)/
/D.Yong and D. L. Lambert(2003)/
/R.G.Gratton et al.(2003)/
/R.Smiljanic et al.(2009)/
/M.Ishigaki et al.(2010)/
/I.U.Roederer et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/K.A.Venn et al.(2004)/

G.S.Bai et al.,AAP, 425, 671, 2004 (A0023,ADS)
Chemical abundances of 10 metal-poor halo stars
Stellar Parameters
Teff : 5090 | log g : 4.60+-0.3 | vturb : 1.50 |
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 | ... | 0.69 | ... | -0.68 | 0.83 | 8.01 | O I |
Na I | N/A | ... | -0.45 | ... | -1.87 | -0.36 | 4.37 | Na I |
Mg I | N/A | ... | 0.22 | ... | -1.31 | 0.20 | 6.29 | Mg I |
Si I | N/A | ... | 0.45 | ... | -1.02 | 0.49 | 6.49 | Si I |
Ca I | N/A | ... | 0.45 | ... | -1.04 | 0.47 | 5.30 | Ca I |
Sc II | N/A | ... | 0.15 | ... | -1.34 | 0.17 | 1.81 | Sc II |
Ti | N/A | ... | 0.36 | ... | -1.08 | 0.43 | 3.87 | Ti |
Cr | N/A | ... | 0.02 | ... | -1.46 | 0.05 | 4.18 | Cr |
Mn I | N/A | ... | -0.23 | ... | -1.78 | -0.27 | 3.65 | Mn I |
Fe I | N/A | -1.51 | ... | ... | -1.51 | ... | 5.99 | Fe I |
Ba II | N/A | ... | 0.28 | ... | -1.28 | 0.23 | 0.90 | Ba II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-04-17 | N/A | PFESSAO | 15000 | 218 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
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 : 5175 | log g : 4.7 | vturb : 0.3 |
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 I | N/A | ... | -0.11 | ... | -1.28 | -0.04 | 4.96 | Na I |
Mg I | N/A | ... | 0.41 | ... | -0.87 | 0.37 | 6.73 | Mg I |
Al I | N/A | ... | 0.2 | ... | -1.04 | 0.20 | 5.41 | Al I |
Si I | N/A | ... | 0.35 | ... | -0.87 | 0.37 | 6.64 | Si I |
Ca I | N/A | ... | 0.27 | ... | -0.97 | 0.27 | 5.37 | Ca I |
Ti | N/A | ... | 0.39 | ... | -0.83 | 0.41 | 4.12 | Ti |
V I | N/A | ... | 0.14 | ... | -1.05 | 0.19 | 2.88 | V I |
Cr I | N/A | ... | 0.06 | ... | -1.17 | 0.07 | 4.47 | Cr I |
Fe | N/A | -1.26 | ... | ... | -1.24 | ... | 6.26 | Fe |
Y II | N/A | ... | 0.37 | ... | -0.86 | 0.38 | 1.35 | Y II |
Zr II | N/A | ... | 0.64 | ... | -0.60 | 0.64 | 1.98 | Zr II |
Ba II | N/A | ... | 0.06 | ... | -1.25 | -0.01 | 0.93 | Ba II |
Eu II | N/A | ... | 0.5 | ... | -0.77 | 0.47 | -0.25 | Eu II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1995-06-10 | N/A | LICKHAMILTON | 50000 | 105 | 2000 | 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
Stellar Parameters
Teff : 4966 | log g : 4.26 | vturb : 0.80 |
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 | ... | -0.05 | ... | ... | ... | C |
Fe I | 16 | -1.54 | ... | ... | ... | ... | Fe I |
Fe II | 9 | -1.44 | ... | ... | ... | ... | Fe 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 |
D.Yong et al.,ApJ, 599, 1357, 2003 (A0133,ADS)
Magnesium Isotopic Abundance Ratios in Cool Stars
Stellar Parameters
Teff : 4950+-150 | log g : 4.50+-0.3 | vturb : 0.3+-0.3 |
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 | -1.46+-0.2 | ... | ... | ... | ... | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | MCDONALD | 60000 | 90 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -041345 | Right Ascension : 163442 |
R.G.Gratton et al.,AAP, 404, 187, 2003 (A0135,ADS)
Abundances for metal-poor stars with accurate parallaxes
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 |
Na I | N/A | ... | 0.07+-0.054 | ... | -1.34+-0.054 | 0.05+-0.054 | 4.90+-0.054 | Na I |
Mg I | N/A | ... | 0.62+-0.055 | ... | -0.93+-0.055 | 0.46+-0.055 | 6.67+-0.055 | Mg I |
Si I | N/A | ... | 0.46+-0.048 | ... | -0.90+-0.048 | 0.49+-0.048 | 6.61+-0.048 | Si I |
Ca I | N/A | ... | 0.36+-0.033 | ... | -1.09+-0.033 | 0.30+-0.033 | 5.25+-0.033 | Ca I |
Ti I | N/A | ... | 0.35+-0.03 | ... | -0.91+-0.03 | 0.48+-0.03 | 4.04+-0.03 | Ti I |
Ti II | N/A | ... | 0.31+-0.048 | ... | -0.95+-0.048 | 0.44+-0.048 | 4.00+-0.048 | Ti II |
Fe I | N/A | -1.38+-0.051 | ... | ... | -1.39+-0.051 | ... | 6.11+-0.051 | Fe I |
Fe II | N/A | -1.34+-0.066 | ... | ... | -1.35+-0.066 | ... | 6.15+-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 | -169.9 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -41344 | Right Ascension : 163443 |
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 : 5175 | log g : 4.64 | vturb : 0.3 |
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 |
Li | N/A | ... | ... | <0.30 | <-2.96 | <-1.86 | <0.30 | Li |
Be | N/A | ... | ... | 0.58 | -0.80 | 0.30 | 0.58 | Be |
Fe | N/A | -1.1 | ... | ... | -1.10 | ... | 6.40 | Fe |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
M.Ishigaki et al.,PASJ, 62, 143, 2010 (A0229,ADS)
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 5515+-69 | log g : 5.00 | vturb : 0.05 |
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 | -1.12+-0.05 | -0.22+-0.05 | ... | ... | Na I |
Mg I | N/A | -0.34+-0.05 | 0.57+-0.05 | ... | ... | Mg I |
Si | N/A | ... | 0.14+-0.05 | ... | ... | ... | Si |
Si I | 2 | -0.77+-0.05 | ... | ... | ... | ... | Si I |
Ca I | N/A | -0.64+-0.05 | 0.26+-0.05 | ... | ... | Ca I |
Ti | N/A | ... | 0.45+-0.04 | ... | ... | ... | Ti |
Ti I | 2 | -0.49+-0.05 | ... | ... | ... | ... | Ti I |
Ti II | 2 | -0.43+-0.05 | ... | ... | ... | ... | Ti II |
Cr | N/A | ... | -0.02+-0.02 | ... | ... | ... | Cr |
Cr I | 5 | -0.92+-0.02 | ... | ... | ... | ... | Cr I |
Cr II | 1 | -0.97+-0.05 | ... | ... | ... | ... | Cr II |
Mn I | N/A | -1.35+-0.07 | 0.07+-0.07 | ... | ... | Mn I |
Fe I | 17 | -0.90+-0.01 | ... | ... | ... | ... | Fe I |
Fe II | 3 | -1.15+-0.10 | ... | ... | ... | ... | Fe II |
Ni I | N/A | -0.85+-0.11 | 0.05+-0.11 | ... | ... | Ni I |
Zn I | N/A | -1.09+-0.06 | -0.18+-0.06 | ... | ... | Zn I |
Y II | N/A | -0.67+-0.05 | 0.24+-0.05 | ... | ... | Y II |
Ba II | N/A | -0.72+-0.05 | 0.19+-0.05 | ... | ... | Ba II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-07-27 | N/A | SUBARUHDS | 50000 | 304 | 1800 | -176.2+-0.4 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -041344.3 | Right Ascension : 163442.35 |
I.U.Roederer et al.,ApJ, 724, 975, 2010 (A0243,ADS)
THE UBIQUITY OF THE RAPID NEUTRON-CAPTURE PROCESS
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 | -1.54 | ... | ... | ... | ... | Fe |
Zn I | N/A | ... | ... | 3.4 | ... | ... | Zn I |
Y II | N/A | ... | ... | 0.87 | ... | ... | Y II |
Pb I | N/A | ... | ... | 0.64 | ... | ... | Pb I |
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 |
M.N.Ishigaki et al.,ApJ, 753, 64, 2012 (A0273,ADS)
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. I. Implications of [alpha/Fe] for Star Formation Histories in Their Progenitors
Stellar Parameters
Teff : 5174+-100 | log g : 4.85+-0.3 | vturb : 0.04+-0.3 |
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 |
Mg | N/A | ... | 0.38+-0.12 | ... | ... | ... | Mg |
Si | N/A | ... | 0.43+-0.16 | ... | ... | ... | Si |
Ca | N/A | ... | 0.21+-0.08 | ... | ... | ... | Ca |
Ti I | N/A | ... | 0.32+-0.11 | ... | ... | ... | Ti I |
Ti II | N/A | ... | 0.43+-0.10 | ... | ... | ... | Ti II |
Fe I | N/A | -1.11+-0.21 | ... | ... | ... | ... | Fe I |
Fe II | N/A | -1.14+-0.12 | ... | ... | ... | ... | Fe II |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | SUBARUHDS | 50000 | N/A | N/A | -179.1+-0.3 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : | Right Ascension : |
M.N.Ishigaki et al.,ApJ, 771, 67, 2013 (A0286,ADS)
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 5174 | log g : 4.85 | vturb : 0.04 |
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 | ... | -0.06+-0.1 | ... | ... | ... | Na I |
Sc II | N/A | ... | 0.2+-0.12 | ... | ... | ... | Sc II |
V I | N/A | ... | 0.09+-0.15 | ... | ... | ... | V I |
Cr I | N/A | ... | -0.03+-0.13 | ... | ... | ... | Cr I |
Cr II | N/A | ... | 0.23+-0.09 | ... | ... | ... | Cr II |
Mn I | N/A | ... | -0.04+-0.23 | ... | ... | ... | Mn I |
Fe I | N/A | -1.17+-0.17 | ... | ... | ... | ... | Fe I |
Fe II | N/A | -1.08+-0.16 | ... | ... | ... | ... | Fe II |
Ni I | N/A | ... | 0.04+-0.1 | ... | ... | ... | Ni I |
Cu I | N/A | ... | -0.15+-0.12 | ... | ... | ... | Cu I |
Zn I | N/A | ... | 0.28+-0.14 | ... | ... | ... | Zn I |
Ba II | N/A | ... | 0.28+-0.23 | ... | ... | ... | Ba II |
Nd II | N/A | ... | 0.89+-0.39 | ... | ... | ... | Nd II |
Sm II | N/A | ... | 0.26+-0.15 | ... | ... | ... | Sm II |
Eu II | N/A | ... | 0.23+-0.21 | ... | ... | ... | Eu II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 50000 | N/A | 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 | ... | -0.11 | ... | ... | ... | Na |
Mg | N/A | ... | 0.41 | ... | ... | ... | Mg |
Ca | N/A | ... | 0.27 | ... | ... | ... | Ca |
Ti | N/A | ... | 0.39 | ... | ... | ... | Ti |
Fe | N/A | -1.26 | ... | ... | ... | ... | Fe |
Y | N/A | ... | 0.37 | ... | ... | ... | Y |
Ba | N/A | ... | 0.06 | ... | ... | ... | Ba |
Eu | N/A | ... | 0.5 | ... | ... | ... | Eu |
Observing Log
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -041345 | Right Ascension : 163442.4 |