HD110184
HIP61824 in K.A.Venn+,AJ, 128, 1177, 2004
taken from 11 paper(s):
/D.L.Burris et al.(2000)/
/S.Honda et al.(2004)/
/J.Melendez and B. Barbuy(2002)/
/T.V.Mishenina et al.(2002)/
/T.V.Mishenina and V. V. Kovtyukh(2001)/
/S.Honda et al.(2004)/
/J.P.Fulbright(2000)/
/J.Simmerer et al.(2004)/
/I.U.Roederer et al.(2010)/
/C.J.Hansen et al.(2012)/
/M.Aoki et al.(2017)/
NEUTRON-CAPTURE ELEMENTS IN THE EARLY GALAXY: INSIGHTS FROM A LARGE SAMPLE OF METAL-POOR GIANTS
Stellar Parameters
Teff : 4250 | log g : 0.30 | vturb : 2.10 |
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 |
Fe | N/A | -2.56 | ... | ... | -2.39 | ... | 5.11 | Fe |
Y | N/A | ... | 0.46 | 0.14 | -2.07 | 0.32 | 0.14 | Y |
Zr | N/A | ... | 1.13 | 1.17 | -1.41 | 0.98 | 1.17 | Zr |
Ba | N/A | ... | 0.01 | -0.42 | -2.60 | -0.21 | -0.42 | Ba |
La | N/A | ... | 0.11 | -1.23 | -2.33 | 0.06 | -1.23 | La |
Nd | N/A | ... | 0.29 | -0.77 | -2.19 | 0.20 | -0.77 | Nd |
Eu | N/A | ... | 0.45 | -1.60 | -2.12 | 0.27 | -1.60 | Eu |
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | 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 | MAYALLKPNO | 20000 | 100-200 | N/A | N/A |
Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. II. The r-Process Elements, Including Thorium
Stellar Parameters
Teff : 4240 | log g : 0.3 | vturb : 2.1 |
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 |
CH | N/A | ... | -0.67 | 5.37 | -3.06 | -0.55 | 5.37 | CH |
Mg I | 2 | ... | 0.19+-0.16 | 5.25+-0.16 | -2.35+-0.16 | 0.16+-0.16 | 5.25+-0.16 | Mg I |
Al I | 1 | ... | -0.84+-0.14 | 3.11+-0.14 | -3.34+-0.14 | -0.83+-0.14 | 3.11+-0.14 | Al I |
Si I | 1 | ... | 0.49+-0.14 | 5.52+-0.14 | -1.99+-0.14 | 0.52+-0.14 | 5.52+-0.14 | Si I |
Ca I | 2 | ... | 0.29+-0.08 | 4.13+-0.08 | -2.21+-0.08 | 0.30+-0.08 | 4.13+-0.08 | Ca I |
Sc II | 2 | ... | -0.06+-0.08 | 0.59+-0.08 | -2.56+-0.08 | -0.05+-0.08 | 0.59+-0.08 | Sc II |
Ti | 21 | ... | 0.08+-0.12 | 2.58+-0.12 | -2.37+-0.12 | 0.14+-0.12 | 2.58+-0.12 | Ti |
Cr | 1 | ... | -0.12+-0.14 | 3.03+-0.14 | -2.61+-0.14 | -0.10+-0.14 | 3.03+-0.14 | Cr |
Mn I | 4 | ... | -0.2+-0.19 | 2.67+-0.19 | -2.76+-0.19 | -0.25+-0.19 | 2.67+-0.19 | Mn I |
Fe | 47 | -2.52+-0.11 | ... | 4.99+-0.11 | -2.51+-0.11 | ... | 4.99+-0.11 | Fe |
Co I | 2 | ... | -0.12+-0.14 | 2.28+-0.14 | -2.71+-0.14 | -0.20+-0.14 | 2.28+-0.14 | Co I |
Ni I | 2 | ... | -0.19+-0.14 | 3.54+-0.14 | -2.68+-0.14 | -0.17+-0.14 | 3.54+-0.14 | Ni I |
Cu I | 1 | ... | -0.67+-0.14 | 1.02+-0.14 | -3.17+-0.14 | -0.66+-0.14 | 1.02+-0.14 | Cu I |
Sr II | 2 | ... | -0.06+-0.14 | 0.34+-0.14 | -2.53+-0.14 | -0.02+-0.14 | 0.34+-0.14 | Sr II |
Y II | 5 | ... | -0.11+-0.16 | -0.4+-0.16 | -2.61+-0.16 | -0.10+-0.16 | -0.4+-0.16 | Y II |
Zr II | 3 | ... | 0.16+-0.1 | 0.25+-0.1 | -2.33+-0.1 | 0.18+-0.1 | 0.25+-0.1 | Zr II |
Ba II | 2 | ... | -0.52+-0.14 | -0.82+-0.14 | -3.00+-0.14 | -0.49+-0.14 | -0.82+-0.14 | Ba II |
La II | 5 | ... | -0.46+-0.14 | -1.76+-0.14 | -2.86+-0.14 | -0.35+-0.14 | -1.76+-0.14 | La II |
Ce II | 7 | ... | -0.56+-0.14 | -1.45+-0.14 | -3.03+-0.14 | -0.52+-0.14 | -1.45+-0.14 | Ce II |
Pr II | 1 | ... | -0.6+-0.14 | -2.32+-0.14 | -3.04+-0.14 | -0.53+-0.14 | -2.32+-0.14 | Pr II |
Nd II | 7 | ... | -0.3+-0.14 | -1.33+-0.14 | -2.75+-0.14 | -0.24+-0.14 | -1.33+-0.14 | Nd II |
Sm II | 4 | ... | -0.09+-0.23 | -1.63+-0.23 | -2.59+-0.23 | -0.08+-0.23 | -1.63+-0.23 | Sm II |
Eu II | 3 | ... | 0.06+-0.05 | -1.91+-0.05 | -2.43+-0.05 | 0.08+-0.05 | -1.91+-0.05 | Eu II |
Gd II | 1 | ... | -0.42+-0.14 | -1.85+-0.14 | -2.92+-0.14 | -0.41+-0.14 | -1.85+-0.14 | Gd II |
Tb II | 2 | ... | -0.55+-0.14 | -2.72+-0.14 | -3.04+-0.14 | -0.53+-0.14 | -2.72+-0.14 | Tb II |
Dy II | 4 | ... | -0.09+-0.24 | -1.44+-0.24 | -2.54+-0.24 | -0.03+-0.24 | -1.44+-0.24 | Dy II |
Er II | 3 | ... | -0.2+-0.08 | -1.75+-0.08 | -2.67+-0.08 | -0.16+-0.08 | -1.75+-0.08 | Er II |
Tm II | 2 | ... | -0.35+-0.14 | -2.72+-0.14 | -2.84+-0.14 | -0.33+-0.14 | -2.72+-0.14 | Tm II |
Yb II | 1 | ... | -0.14+-0.14 | -1.7+-0.14 | -2.62+-0.14 | -0.11+-0.14 | -1.7+-0.14 | Yb II |
Th II | 1 | ... | -0.07+-0.15 | -2.5+-0.15 | -2.56+-0.15 | -0.05+-0.15 | -2.5+-0.15 | Th II |
U II | 1 | ... | <0.50 | <-2.52 | <-1.98 | <0.53 | <-2.52 | U II |
Isotopic Ratio
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-01-29 | N/A | SUBARUHDS | 90000 | 221 | 900 | 138.89+-0.27 |
Keck NIRSPEC Infrared OH Lines: Oxygen Abundances in Metal-poor Stars down to [Fe/H] = -2.9
Stellar Parameters
Teff : 4262 | log g : 0.7 | vturb : 2.4 |
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 |
C | N/A | ... | -0.58 | ... | -2.87 | -0.46 | 5.56 | C |
OH | N/A | ... | +0.51 | ... | -1.82 | 0.59 | 6.87 | OH |
Fe II | N/A | -2.41 | ... | ... | -2.41 | ... | 5.09 | Fe II |
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-05-20 | N/A | KECKNIRSPEC | 37000 | 180 | 8x80 | N/A |
2001-01-18 | N/A | FEROSESO | 48000 | 300 | 1800 | N/A |
Abundances of Cu and Zn in metal-poor stars: Clues for Galaxy evolution
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 |
Fe | N/A | -2.27 | ... | ... | -2.27 | ... | 5.23 | Fe |
Cu I | N/A | ... | -0.63+-0.31 | ... | -2.88+-0.31 | -0.61+-0.31 | 1.31+-0.31 | Cu I |
Zn I | N/A | ... | 0.22+-0.24 | ... | -2.01+-0.24 | 0.26+-0.24 | 2.55+-0.24 | Zn I |
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | 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 | ELODIE | 42000 | >100 | N/A | N/A |
Analysis of neutron capture elements in metal-poor stars
Stellar Parameters
Teff : 4380 | log g : 0.6 | vturb : 1.9 |
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 |
Mg I | N/A | ... | 0.25 | ... | -2.04 | 0.23 | 5.56 | Mg I |
Si I | N/A | ... | 0.18 | ... | -2.05 | 0.22 | 5.46 | Si I |
Ca I | N/A | ... | 0.31 | ... | -1.94 | 0.33 | 4.40 | Ca I |
Fe | N/A | -2.27 | ... | ... | -2.27 | ... | 5.23 | Fe |
Sr I | N/A | ... | -0.27 | ... | -2.44 | -0.17 | 0.43 | Sr I |
Ba II | N/A | ... | -0.34 | ... | -2.66 | -0.39 | -0.48 | Ba II |
Ce II | N/A | ... | -0.29 | ... | -2.56 | -0.29 | -0.98 | Ce II |
Nd II | N/A | ... | 0.03 | ... | -2.16 | 0.11 | -0.74 | Nd II |
Eu II | N/A | ... | 0.28 | ... | -2.00 | 0.27 | -1.48 | Eu II |
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | 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 | ELODIE | 42000 | >100 | N/A | N/A |
Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. I. Observational Data
Binary Parameters
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-01-29 | N/A | SUBARUHDS | 90000 | 221 | 900 | 138.89+-0.27 |
ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
Stellar Parameters
Teff : 4400 | log g : 0.6 | vturb : 2.8 |
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 | ... | -0.49 | ... | -2.84 | -0.42 | 3.40 | Na I |
Mg I | N/A | ... | 0.56 | ... | -1.90 | 0.52 | 5.70 | Mg I |
Ca I | N/A | ... | 0.42 | ... | -2.00 | 0.42 | 4.34 | Ca I |
Ti | N/A | ... | 0.29 | ... | -2.11 | 0.31 | 2.84 | Ti |
V I | N/A | ... | -0.07 | ... | -2.44 | -0.02 | 1.49 | V I |
Cr I | N/A | ... | -0.24 | ... | -2.65 | -0.23 | 2.99 | Cr I |
Fe | N/A | -2.44 | ... | ... | -2.42 | ... | 5.08 | Fe |
Ni I | N/A | ... | 0.01 | ... | -2.40 | 0.02 | 3.82 | Ni I |
Y II | N/A | ... | -0.18 | ... | -2.59 | -0.17 | -0.38 | Y II |
Ba II | N/A | ... | -0.4 | ... | -2.89 | -0.47 | -0.71 | Ba II |
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
19990126-31 | N/A | SANDIFORD | 50000 | 75 | 1200 | N/A |
1999046-7 | N/A | LICKHAMILTON | 50000 | 50 | 1800 | N/A |
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 4250 | log g : 0.79 | vturb : 2.50 |
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 |
C | N/A | ... | -0.3 | ... | -2.84 | -0.12 | 5.59 | C |
Fe I | 11 | -2.72 | ... | ... | -2.72 | ... | 4.78 | Fe I |
Fe II | 6 | -2.50 | ... | ... | -2.50 | ... | 5.00 | Fe II |
La II | N/A | ... | ... | -1.47+-0.03 | -2.57+-0.03 | 0.15+-0.03 | -1.47+-0.03 | La II |
Eu II | N/A | ... | ... | -1.71+-0.09 | -2.23+-0.09 | 0.49+-0.09 | -1.71+-0.09 | Eu II |
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | 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 | MCDONALD | 60000 | 100 | N/A | N/A |
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 | -2.72 | ... | ... | -2.72 | ... | 4.78 | Fe |
Zn I | N/A | ... | ... | 2.14 | -2.42 | 0.30 | 2.14 | Zn I |
Y II | N/A | ... | ... | -0.65 | -2.86 | -0.14 | -0.65 | Y II |
Pb I | N/A | ... | ... | <-0.20 | <-2.24 | <0.48 | <-0.20 | Pb I |
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | 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 | MCDONALD | 60000 | 100 | N/A | N/A |
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
Teff : 4450+-100 | log g : 0.50+-0.25 | vturb : 2.1+-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 | -2.40+-0.15 | ... | ... | -2.40+-0.15 | ... | 5.10+-0.15 | Fe |
Sr | N/A | ... | -0.05+-0.22 | ... | -2.45+-0.22 | -0.05+-0.22 | 0.42+-0.22 | Sr |
Y | N/A | ... | 0.15+-0.14 | ... | -2.25+-0.14 | 0.15+-0.14 | -0.04+-0.14 | Y |
Zr | N/A | ... | 0.47+-0.18 | ... | -1.93+-0.18 | 0.47+-0.18 | 0.65+-0.18 | Zr |
Pd | N/A | ... | 0.22+-0.23 | ... | -2.18+-0.23 | 0.22+-0.23 | -0.61+-0.23 | Pd |
Ag | N/A | ... | 0.15+-0.22 | ... | -2.51+-0.22 | -0.11+-0.22 | -1.31+-0.22 | Ag |
Ba | N/A | ... | -0.06+-0.14 | ... | -2.46+-0.14 | -0.06+-0.14 | -0.28+-0.14 | Ba |
Eu | N/A | ... | 0.22+-0.16 | ... | -2.18+-0.16 | 0.22+-0.16 | -1.66+-0.16 | Eu |
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | 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 |
Diversity of Abundance Patterns of Light Neutron-capture Elements in Very-metal-poor Stars
Stellar Parameters
Teff : 4240 | log g : 0.30 | vturb : 2.21 |
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 | -2.52 | ... | ... | -2.52 | ... | 4.98 | Fe |
Sr II | 1 | ... | 0.11+-0.28 | 0.46+-0.28 | -2.41+-0.28 | 0.11+-0.28 | 0.46+-0.28 | Sr II |
Y II | 4 | ... | -0.51+-0.18 | -0.82+-0.18 | -3.03+-0.18 | -0.51+-0.18 | -0.82+-0.18 | Y II |
Zr II | 6 | ... | -0.13+-0.21 | -0.07+-0.21 | -2.65+-0.21 | -0.13+-0.21 | -0.07+-0.21 | Zr II |
Mo I | 1 | ... | -0.06+-0.17 | -0.70+-0.17 | -2.58+-0.17 | -0.06+-0.17 | -0.70+-0.17 | Mo I |
Ru I | 2 | ... | -0.08+-0.21 | -0.85+-0.21 | -2.60+-0.21 | -0.08+-0.21 | -0.85+-0.21 | Ru I |
Pd I | 1 | ... | -0.27+-0.18 | -1.22+-0.18 | -2.79+-0.18 | -0.27+-0.18 | -1.22+-0.18 | Pd I |
Ba II | 4 | ... | -0.72+-0.18 | -1.06+-0.18 | -3.24+-0.18 | -0.72+-0.18 | -1.06+-0.18 | Ba II |
La II | 4 | ... | -0.31+-0.16 | -1.73+-0.16 | -2.83+-0.16 | -0.31+-0.16 | -1.73+-0.16 | La II |
Ce II | 5 | ... | -0.32+-0.16 | -1.26+-0.16 | -2.84+-0.16 | -0.32+-0.16 | -1.26+-0.16 | Ce II |
Nd II | 3 | ... | -0.20+-0.16 | -1.30+-0.16 | -2.72+-0.16 | -0.20+-0.16 | -1.30+-0.16 | Nd II |
Eu II | 2 | ... | -0.03+-0.16 | -2.03+-0.16 | -2.55+-0.16 | -0.03+-0.16 | -2.03+-0.16 | Eu II |
Binary Parameters
Position
Right Ascension : 12 40 14.08 | Declination : +08 31 38.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2007-02-08 | N/A | SUBARUHDS | 90000 | 630 | 20400 | 139.5+-0.6 |