G59-27
taken from 6 paper(s):
/P.E.Nissen et al.(2007)/
/M.Ishigaki et al.(2010)/
/D.Fabbian et al.(2009)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/A.M.Amarsi et al.(2019)/
Sulphur and zinc abundances in Galactic halo stars revisited
Stellar Parameters
Teff : 6272 | log g : 4.23 | 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 |
S I | N/A | ... | 0.30 | ... | -1.42 | 0.51 | 5.70 | S I |
Fe | N/A | -1.93 | ... | ... | -1.93 | ... | 5.57 | Fe |
Zn I | N/A | ... | 0.06 | 2.73 | -1.83 | 0.10 | 2.73 | Zn I |
Position
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 |
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 5829+-108 | log g : 3.20 | vturb : 1.66 |
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 | -1.69+-0.04 | 0.73+-0.04 | ... | -1.71+-0.04 | 0.71+-0.04 | 5.89+-0.04 | Mg I |
Ca I | N/A | -1.93+-0.02 | 0.49+-0.02 | ... | -1.91+-0.02 | 0.51+-0.02 | 4.43+-0.02 | Ca I |
Ti | N/A | ... | 0.39+-0.03 | ... | -1.96+-0.03 | 0.46+-0.03 | 2.99+-0.03 | Ti |
Ti I | 1 | -2.04+-0.06 | ... | ... | -1.97+-0.06 | 0.45+-0.06 | 2.98+-0.06 | Ti I |
Ti II | 5 | -2.02+-0.04 | ... | ... | -1.95+-0.04 | 0.47+-0.04 | 3.00+-0.04 | Ti II |
Mn I | N/A | -2.88+-0.05 | 0.06+-0.06 | ... | -2.92+-0.05 | -0.50+-0.06 | 2.51+-0.05 | Mn I |
Fe I | 21 | -2.42+-0.01 | ... | ... | -2.42+-0.01 | ... | 5.08+-0.01 | Fe I |
Fe II | 5 | -2.40+-0.03 | ... | ... | -2.40+-0.03 | ... | 5.10+-0.03 | Fe II |
Y II | N/A | -2.57+-0.06 | -0.15+-0.06 | ... | -2.54+-0.06 | -0.12+-0.06 | -0.33+-0.06 | Y II |
Ba II | N/A | -2.90+-0.06 | -0.48+-0.06 | ... | -2.95+-0.06 | -0.53+-0.06 | -0.77+-0.06 | Ba II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-07-27 | N/A | SUBARUHDS | 50000 | 155 | 2700 | -120.2+-0.4 |
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 | -1.58 | ... | 6.81 | -1.62 | 0.36 | 6.81 | C |
O | N/A | -1.06 | ... | 7.60 | -1.09 | 0.89 | 7.60 | O |
Fe | N/A | -1.93 | ... | ... | -1.98 | ... | 5.52 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004 | N/A | VLT | 60000 | 70-170 | 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 : 6297+-100 | log g : 4.12+-0.3 | vturb : 1.16+-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 | ... | 0.28+-0.07 | ... | -1.71+-0.07 | 0.28+-0.07 | 5.89+-0.07 | Mg |
Ca | N/A | ... | 0.38+-0.08 | ... | -1.61+-0.08 | 0.38+-0.08 | 4.73+-0.08 | Ca |
Ti I | N/A | ... | 0.43+-0.07 | ... | -1.56+-0.07 | 0.43+-0.07 | 3.39+-0.07 | Ti I |
Ti II | N/A | ... | 0.48+-0.09 | ... | -1.51+-0.09 | 0.48+-0.09 | 3.44+-0.09 | Ti II |
Fe I | N/A | -1.99+-0.09 | ... | ... | -1.99+-0.09 | ... | 5.51+-0.09 | Fe I |
Fe II | N/A | -1.99+-0.12 | ... | ... | -1.99+-0.12 | ... | 5.51+-0.12 | Fe II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | SUBARUHDS | 50000 | N/A | N/A | -119.2+-0.3 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 6297 | log g : 4.12 | vturb : 1.16 |
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 |
Sc II | N/A | ... | 0.13+-0.13 | ... | -1.86+-0.13 | 0.13+-0.13 | 1.29+-0.13 | Sc II |
Cr I | N/A | ... | -0.1+-0.07 | ... | -2.09+-0.07 | -0.10+-0.07 | 3.55+-0.07 | Cr I |
Cr II | N/A | ... | 0.15+-0.1 | ... | -1.84+-0.1 | 0.15+-0.1 | 3.80+-0.1 | Cr II |
Mn I | N/A | ... | -0.38+-0.1 | ... | -2.37+-0.1 | -0.38+-0.1 | 3.06+-0.1 | Mn I |
Fe I | N/A | -1.99+-0.09 | ... | ... | -1.99+-0.09 | ... | 5.51+-0.09 | Fe I |
Fe II | N/A | -1.99+-0.12 | ... | ... | -1.99+-0.12 | ... | 5.51+-0.12 | Fe II |
Co I | N/A | ... | 0.09+-0.11 | ... | -1.90+-0.11 | 0.09+-0.11 | 3.09+-0.11 | Co I |
Cu I | N/A | ... | -2.19 | ... | -4.18 | -2.19 | 0.01 | Cu I |
Sr II | N/A | ... | 0.13+-0.23 | ... | -1.86+-0.23 | 0.13+-0.23 | 1.01+-0.23 | Sr II |
Ba II | N/A | ... | -0.17+-0.11 | ... | -2.16+-0.11 | -0.17+-0.11 | 0.02+-0.11 | Ba II |
Eu II | N/A | ... | 0.07 | ... | -1.92 | 0.07 | -1.40 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 50000 | N/A | N/A | N/A |
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 | ... | 0.25 | ... | -1.64 | 0.25 | 6.79 | C |
O | N/A | ... | 0.79 | ... | -1.10 | 0.79 | 7.59 | O |
Fe | N/A | -1.89 | ... | ... | -1.89 | ... | 5.61 | Fe |
Position
Right Ascension : 12 36 39.45 | Declination : +27 28 28.16 | 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 |