G23-14
taken from 4 paper(s):
/J.Simmerer et al.(2004)/
/I.U.Roederer et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 5025 | log g : 4.02 | vturb : 1.30 |
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 | ... | -0.2 | ... | -1.66 | -0.02 | 6.77 | C |
Fe I | 15 | -1.64 | ... | ... | -1.64 | ... | 5.86 | Fe I |
Fe II | 7 | -1.57 | ... | ... | -1.57 | ... | 5.93 | Fe II |
La II | N/A | ... | ... | -0.33+-0.04 | -1.43+-0.04 | 0.21+-0.04 | -0.33+-0.04 | La II |
Eu II | N/A | ... | ... | -0.58+-0.12 | -1.10+-0.12 | 0.54+-0.12 | -0.58+-0.12 | Eu II |
Position
Right Ascension : 19 51 49.61 | Declination : +05 36 45.8 | 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 | -1.64 | ... | ... | -1.64 | ... | 5.86 | Fe |
Zn I | N/A | ... | ... | 3.05 | -1.51 | 0.13 | 3.05 | Zn I |
Y II | N/A | ... | ... | 0.46 | -1.75 | -0.11 | 0.46 | Y II |
Pb I | N/A | ... | ... | <+0.75 | <-1.29 | <0.35 | <+0.75 | Pb I |
Position
Right Ascension : 19 51 49.61 | Declination : +05 36 45.8 | 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 |
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 : 5061+-100 | log g : 3.08+-0.3 | vturb : 1.10+-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 | ... | 0.29+-0.11 | ... | -1.18+-0.11 | 0.29+-0.11 | 6.42+-0.11 | Mg |
Si | N/A | ... | 0.27+-0.15 | ... | -1.20+-0.15 | 0.27+-0.15 | 6.31+-0.15 | Si |
Ca | N/A | ... | 0.30+-0.08 | ... | -1.17+-0.08 | 0.30+-0.08 | 5.17+-0.08 | Ca |
Ti I | N/A | ... | 0.19+-0.07 | ... | -1.28+-0.07 | 0.19+-0.07 | 3.67+-0.07 | Ti I |
Ti II | N/A | ... | 0.30+-0.09 | ... | -1.17+-0.09 | 0.30+-0.09 | 3.78+-0.09 | Ti II |
Fe I | N/A | -1.47+-0.15 | ... | ... | -1.47+-0.15 | ... | 6.03+-0.15 | Fe I |
Fe II | N/A | -1.47+-0.14 | ... | ... | -1.47+-0.14 | ... | 6.03+-0.14 | Fe II |
Binary Parameters
Position
Right Ascension : 19 51 49.61 | Declination : +05 36 45.8 | 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 | SUBARUHDS | 50000 | N/A | N/A | 13.2+-0.4 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 5061 | log g : 3.08 | vturb : 1.1 |
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 |
Na I | N/A | ... | -0.11+-0.12 | ... | -1.59+-0.12 | -0.11+-0.12 | 4.65+-0.12 | Na I |
Sc II | N/A | ... | 0.06+-0.07 | ... | -1.42+-0.07 | 0.06+-0.07 | 1.73+-0.07 | Sc II |
V I | N/A | ... | 0.11+-0.19 | ... | -1.37+-0.19 | 0.11+-0.19 | 2.56+-0.19 | V I |
Cr I | N/A | ... | -0.13+-0.06 | ... | -1.61+-0.06 | -0.13+-0.06 | 4.03+-0.06 | Cr I |
Cr II | N/A | ... | 0.23+-0.08 | ... | -1.25+-0.08 | 0.23+-0.08 | 4.39+-0.08 | Cr II |
Mn I | N/A | ... | -0.27+-0.07 | ... | -1.75+-0.07 | -0.27+-0.07 | 3.68+-0.07 | Mn I |
Fe I | N/A | -1.48+-0.15 | ... | ... | -1.48+-0.15 | ... | 6.02+-0.15 | Fe I |
Fe II | N/A | -1.46+-0.14 | ... | ... | -1.46+-0.14 | ... | 6.04+-0.14 | Fe II |
Ni I | N/A | ... | -0.08+-0.09 | ... | -1.56+-0.09 | -0.08+-0.09 | 4.66+-0.09 | Ni I |
Cu I | N/A | ... | -0.72+-0.12 | ... | -2.20+-0.12 | -0.72+-0.12 | 1.99+-0.12 | Cu I |
Zn I | N/A | ... | 0.1+-0.17 | ... | -1.38+-0.17 | 0.10+-0.17 | 3.18+-0.17 | Zn I |
Y II | N/A | ... | -0.13+-0.08 | ... | -1.61+-0.08 | -0.13+-0.08 | 0.60+-0.08 | Y II |
Ba II | N/A | ... | 0.05+-0.18 | ... | -1.43+-0.18 | 0.05+-0.18 | 0.75+-0.18 | Ba II |
Nd II | N/A | ... | 0.24+-0.12 | ... | -1.24+-0.12 | 0.24+-0.12 | 0.18+-0.12 | Nd II |
Sm II | N/A | ... | 0.33+-0.1 | ... | -1.15+-0.1 | 0.33+-0.1 | -0.19+-0.1 | Sm II |
Eu II | N/A | ... | 0.42+-0.07 | ... | -1.06+-0.07 | 0.42+-0.07 | -0.54+-0.07 | Eu II |
Position
Right Ascension : 19 51 49.61 | Declination : +05 36 45.8 | 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 | SUBARUHDS | 50000 | N/A | N/A | N/A |