G53-41
taken from 13 paper(s):
/P.E.Nissen et al.(2007)/
/C.J.Akerman et al.(2004)/
/J.Melendez et al.(2006)/
/P.E.Nissen et al.(2004)/
/M.Ishigaki et al.(2010)/
/J.Melendez et al.(2010)/
/D.Fabbian et al.(2009)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/L.Zhang et al.(2009)/
/A.M.Amarsi et al.(2019)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
Sulphur and zinc abundances in Galactic halo stars revisited
Stellar Parameters
Teff : 5993 | log g : 4.22 | 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 |
S I | N/A | ... | 0.27 | ... | -0.81 | 0.48 | 6.31 | S I |
Fe | N/A | -1.29 | ... | ... | -1.29 | ... | 6.21 | Fe |
Zn I | N/A | ... | 0.02 | 3.33 | -1.23 | 0.06 | 3.33 | Zn I |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2007-06-25 | N/A | VLT | 60000 | N/A | N/A | N/A |
The evolution of the C/O ratio in metal-poor halo stars
Stellar Parameters
Teff : 5829 | log g : 4.15 | 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 |
C I | N/A | ... | ... | 7.07 | -1.36 | -0.02 | 7.07 | C I |
O I | N/A | ... | ... | 7.86 | -0.83 | 0.51 | 7.86 | O I |
Fe | N/A | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | 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 | 60000 | 200-300 | 3600 | N/A |
PERMITTED OXYGEN ABUNDANCES AND THE TEMPERATURE SCALE OF METAL-POOR TURNOFF STARS
Stellar Parameters
Teff : 5970+-27 | log g : 4.38+-0.15 | 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 |
O I | N/A | ... | ... | 7.89 | -0.80 | 0.46 | 7.89 | O I |
Fe II | N/A | ... | ... | 6.24 | -1.26 | ... | 6.24 | Fe II |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | 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 | 60000 | 200-300 | N/A | N/A |
Sulphur and zinc abundances in Galactic stars and damped Ly alpha systems
Stellar Parameters
Teff : 5829+-70 | log g : 4.15+-0.15 | vturb : 1.3+-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 |
S I | N/A | -1.05 | ... | ... | -0.97 | 0.37 | 6.15 | S I |
Fe II | N/A | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe II |
Zn I | N/A | -1.29 | ... | ... | -1.28 | 0.06 | 3.28 | Zn I |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001 | N/A | VLT | 60000 | 150-300 | N/A | N/A |
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 5737+-68 | log g : 4.12 | 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 |
Na I | N/A | -1.26+-0.04 | 0.18+-0.05 | ... | -1.17+-0.04 | 0.27+-0.05 | 5.07+-0.04 | Na I |
Mg I | N/A | -1.12+-0.05 | 0.32+-0.06 | ... | -1.14+-0.05 | 0.30+-0.06 | 6.46+-0.05 | Mg I |
Si | N/A | ... | 0.39+-0.07 | ... | -1.01+-0.07 | 0.43+-0.07 | 6.50+-0.07 | Si |
Si I | 2 | -1.15+-0.10 | ... | ... | -1.11+-0.10 | 0.33+-0.10 | 6.40+-0.10 | Si I |
Si II | 1 | -0.95+-0.10 | ... | ... | -0.91+-0.10 | 0.53+-0.10 | 6.60+-0.10 | Si II |
Ca I | N/A | -1.18+-0.03 | 0.25+-0.03 | ... | -1.16+-0.03 | 0.28+-0.03 | 5.18+-0.03 | Ca I |
Ti | N/A | ... | 0.24+-0.02 | ... | -1.13+-0.02 | 0.31+-0.02 | 3.82+-0.02 | Ti |
Ti I | 6 | -1.29+-0.03 | ... | ... | -1.22+-0.03 | 0.22+-0.03 | 3.73+-0.03 | Ti I |
Ti II | 10 | -1.05+-0.03 | ... | ... | -0.98+-0.03 | 0.46+-0.03 | 3.97+-0.03 | Ti II |
Cr | N/A | ... | -0.17+-0.03 | ... | -1.58+-0.03 | -0.14+-0.03 | 4.06+-0.03 | Cr |
Cr I | 7 | -1.62+-0.02 | ... | ... | -1.59+-0.02 | -0.15+-0.02 | 4.05+-0.02 | Cr I |
Cr II | 2 | -1.34+-0.10 | ... | ... | -1.31+-0.10 | 0.13+-0.10 | 4.33+-0.10 | Cr II |
Mn I | N/A | -1.96+-0.10 | 0.10+-0.10 | ... | -2.00+-0.10 | -0.56+-0.10 | 3.43+-0.10 | Mn I |
Fe I | 56 | -1.44+-0.02 | ... | ... | -1.44+-0.02 | ... | 6.06+-0.02 | Fe I |
Fe II | 10 | -1.44+-0.03 | ... | ... | -1.44+-0.03 | ... | 6.06+-0.03 | Fe II |
Ni I | N/A | -1.50+-0.02 | -0.06+-0.03 | ... | -1.47+-0.02 | -0.03+-0.03 | 4.75+-0.02 | Ni I |
Zn I | N/A | -1.49+-0.10 | -0.06+-0.10 | ... | -1.45+-0.10 | -0.01+-0.10 | 3.11+-0.10 | Zn I |
Y II | N/A | -1.31+-0.10 | 0.13+-0.10 | ... | -1.28+-0.10 | 0.16+-0.10 | 0.93+-0.10 | Y II |
Ba II | N/A | -1.21+-0.12 | 0.23+-0.12 | ... | -1.26+-0.12 | 0.18+-0.12 | 0.92+-0.12 | Ba II |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-07-27 | N/A | SUBARUHDS | 50000 | >100 | N/A | N/A |
Observational evidence for a broken Li Spite plateau and mass-dependent Li depletion
Stellar Parameters
Teff : 6049+-50 | log g : 4.31 |
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 | ... | ... | 2.14+-0.035 | -1.12+-0.035 | 0.12+-0.035 | 2.14+-0.035 | Li |
Fe | N/A | -1.24 | ... | ... | -1.24 | ... | 6.26 | Fe |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | 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 | FIESNOT | 45000 | >100 | N/A | N/A |
The C/O ratio at low metallicity:constraints on early chemical evolution from observations of Galactic halo stars
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 |
C | N/A | -1.38 | ... | 7.01 | -1.42 | -0.08 | 7.01 | C |
O | N/A | -0.88 | ... | 7.78 | -0.91 | 0.43 | 7.78 | O |
Fe | N/A | -1.29 | ... | ... | -1.34 | ... | 6.16 | Fe |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001 | N/A | VLT | 60000 | N/A | 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 : 6070+-100 | log g : 4.56+-0.3 | vturb : 0.77+-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 | ... | 0.16+-0.13 | ... | -0.98+-0.13 | 0.16+-0.13 | 6.62+-0.13 | Mg |
Si | N/A | ... | 0.13+-0.14 | ... | -1.01+-0.14 | 0.13+-0.14 | 6.50+-0.14 | Si |
Ca | N/A | ... | 0.21+-0.07 | ... | -0.93+-0.07 | 0.21+-0.07 | 5.41+-0.07 | Ca |
Ti I | N/A | ... | 0.27+-0.07 | ... | -0.87+-0.07 | 0.27+-0.07 | 4.08+-0.07 | Ti I |
Ti II | N/A | ... | 0.32+-0.08 | ... | -0.82+-0.08 | 0.32+-0.08 | 4.13+-0.08 | Ti II |
Fe I | N/A | -1.14+-0.12 | ... | ... | -1.14+-0.12 | ... | 6.36+-0.12 | Fe I |
Fe II | N/A | -1.15+-0.11 | ... | ... | -1.15+-0.11 | ... | 6.35+-0.11 | Fe II |
Binary Parameters
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | 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 | 84.8+-0.5 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 6070 | log g : 4.56 | vturb : 0.77 |
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 | ... | 0.1+-0.1 | ... | -1.04+-0.1 | 0.10+-0.1 | 5.20+-0.1 | Na I |
Sc II | N/A | ... | 0.1+-0.07 | ... | -1.04+-0.07 | 0.10+-0.07 | 2.11+-0.07 | Sc II |
V I | N/A | ... | 0.02+-0.14 | ... | -1.12+-0.14 | 0.02+-0.14 | 2.81+-0.14 | V I |
Cr I | N/A | ... | -0.09+-0.07 | ... | -1.23+-0.07 | -0.09+-0.07 | 4.41+-0.07 | Cr I |
Cr II | N/A | ... | 0.17+-0.09 | ... | -0.97+-0.09 | 0.17+-0.09 | 4.67+-0.09 | Cr II |
Mn I | N/A | ... | -0.32+-0.08 | ... | -1.46+-0.08 | -0.32+-0.08 | 3.97+-0.08 | Mn I |
Fe I | N/A | -1.14+-0.12 | ... | ... | -1.14+-0.12 | ... | 6.36+-0.12 | Fe I |
Fe II | N/A | -1.15+-0.11 | ... | ... | -1.15+-0.11 | ... | 6.35+-0.11 | Fe II |
Ni I | N/A | ... | -0.14+-0.09 | ... | -1.28+-0.09 | -0.14+-0.09 | 4.94+-0.09 | Ni I |
Cu I | N/A | ... | -0.75+-0.12 | ... | -1.89+-0.12 | -0.75+-0.12 | 2.30+-0.12 | Cu I |
Zn I | N/A | ... | 0.04+-0.12 | ... | -1.10+-0.12 | 0.04+-0.12 | 3.46+-0.12 | Zn I |
Y II | N/A | ... | 0.1+-0.09 | ... | -1.04+-0.09 | 0.10+-0.09 | 1.17+-0.09 | Y II |
Ba II | N/A | ... | 0.54+-0.15 | ... | -0.60+-0.15 | 0.54+-0.15 | 1.58+-0.15 | Ba II |
La II | N/A | ... | 0.57+-0.12 | ... | -0.57+-0.12 | 0.57+-0.12 | 0.53+-0.12 | La II |
Nd II | N/A | ... | 0.61+-0.12 | ... | -0.53+-0.12 | 0.61+-0.12 | 0.89+-0.12 | Nd II |
Eu II | N/A | ... | 0.49+-0.07 | ... | -0.65+-0.07 | 0.49+-0.07 | -0.13+-0.07 | Eu II |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | 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 |
Chemical Compositions of Kinematically Selected Outer Halo Stars
Stellar Parameters
Teff : 5840+-80 | log g : 4.51+-0.24 | vturb : 1.10+-0.1 |
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 | 2 | -0.97+-0.08 | 0.25+-0.08 | ... | -0.88+-0.08 | 0.17+-0.08 | 5.36+-0.08 | Na I |
Mg I | 1 | -1.00+-0.08 | 0.22+-0.08 | ... | -1.02+-0.08 | 0.03+-0.08 | 6.58+-0.08 | Mg I |
Si | N/A | ... | 0.23+-0.07 | ... | -0.95+-0.07 | 0.10+-0.07 | 6.56+-0.07 | Si |
Si I | 2 | -0.99+-0.07 | ... | ... | -0.95+-0.07 | 0.10+-0.07 | 6.56+-0.07 | Si I |
Si II | 1 | -0.89+-0.04 | ... | ... | -0.85+-0.04 | 0.20+-0.04 | 6.66+-0.04 | Si II |
Ca I | 22 | -1.02+-0.06 | 0.20+-0.06 | ... | -1.00+-0.06 | 0.05+-0.06 | 5.34+-0.06 | Ca I |
Sc II | 8 | -1.04+-0.07 | 0.18+-0.07 | ... | -1.10+-0.07 | -0.05+-0.07 | 2.05+-0.07 | Sc II |
Ti | N/A | ... | 0.26+-0.08 | ... | -0.92+-0.08 | 0.13+-0.08 | 4.03+-0.08 | Ti |
Ti I | 29 | -0.96+-0.08 | ... | ... | -0.92+-0.08 | 0.13+-0.08 | 4.03+-0.08 | Ti I |
Ti II | 11 | -0.80+-0.08 | ... | ... | -0.76+-0.08 | 0.29+-0.08 | 4.19+-0.08 | Ti II |
Cr | N/A | ... | -0.13+-0.06 | ... | -1.32+-0.06 | -0.27+-0.06 | 4.32+-0.06 | Cr |
Cr I | 14 | -1.35+-0.06 | ... | ... | -1.32+-0.06 | -0.27+-0.06 | 4.32+-0.06 | Cr I |
Cr II | 5 | -1.03+-0.09 | ... | ... | -1.00+-0.09 | 0.05+-0.09 | 4.64+-0.09 | Cr II |
Mn I | 2 | -1.62+-0.03 | -0.41+-0.03 | ... | -1.66+-0.03 | -0.61+-0.03 | 3.77+-0.03 | Mn I |
Fe | N/A | -1.22+-0.05 | ... | ... | -1.05+-0.05 | ... | 6.45+-0.05 | Fe |
Fe I | 93 | -1.22+-0.05 | ... | ... | -1.05+-0.05 | ... | 6.45+-0.05 | Fe I |
Fe II | 12 | -1.22+-0.06 | ... | ... | -1.05+-0.06 | ... | 6.45+-0.06 | Fe II |
Ni I | 17 | -1.29+-0.07 | -0.07+-0.07 | ... | -1.26+-0.07 | -0.21+-0.07 | 4.96+-0.07 | Ni I |
Zn I | 3 | -1.28+-0.05 | -0.06+-0.05 | ... | -1.24+-0.05 | -0.19+-0.05 | 3.32+-0.05 | Zn I |
Y II | 2 | -1.12+-0.05 | 0.10+-0.05 | ... | -1.09+-0.05 | -0.04+-0.05 | 1.12+-0.05 | Y II |
Ba II | 3 | -0.95+-0.06 | 0.27+-0.06 | ... | -1.00+-0.06 | 0.05+-0.06 | 1.18+-0.06 | Ba II |
Binary Parameters
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | 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 | 1800 | 88.2 |
Carbon and oxygen in metal-poor halo stars
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 |
C | N/A | ... | -0.20 | ... | -1.35 | -0.20 | 7.08 | C |
O | N/A | ... | 0.32 | ... | -0.83 | 0.32 | 7.86 | O |
Fe | N/A | -1.15 | ... | ... | -1.15 | ... | 6.35 | Fe |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.18 | 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 | VLT | 60000 | 15-300 | N/A | N/A |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5859 | log g : 4.27 | 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 | ... | 0.23 | ... | -0.88 | 0.32 | 5.36 | Na |
Mg | N/A | ... | 0.24 | ... | -0.98 | 0.22 | 6.62 | Mg |
Si | N/A | ... | 0.24 | ... | -0.92 | 0.28 | 6.59 | Si |
Ca | N/A | ... | 0.31 | ... | -0.87 | 0.33 | 5.47 | Ca |
Ti | N/A | ... | 0.14 | ... | -0.99 | 0.21 | 3.96 | Ti |
Cr | N/A | ... | -0.03 | ... | -1.20 | 0.00 | 4.44 | Cr |
Fe | N/A | -1.20 | ... | ... | -1.20 | ... | 6.30 | Fe |
Ni | N/A | ... | -0.09 | ... | -1.26 | -0.06 | 4.96 | Ni |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-12-04-0541 | N/A | FIESNOT | 40000 | 180 | N/A | 88.4 |
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 | ... | -0.38 | ... | -1.62 | -0.42 | 3.81 | Mn |
Fe | N/A | -1.2 | ... | ... | -1.20 | ... | 6.30 | Fe |
Zn | N/A | ... | 0.03 | ... | -1.13 | 0.07 | 3.43 | Zn |
Y | N/A | ... | 0.05 | ... | -1.12 | 0.08 | 1.09 | Y |
Ba | N/A | ... | 0.24 | ... | -1.01 | 0.19 | 1.17 | Ba |
Position
Right Ascension : 10 27 24.25 | Declination : +01 24 00.2 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-12-04-0541 | N/A | FIESNOT | 40000 | 180 | N/A | 88.4 |