G64-12
taken from 34 paper(s):
/G.Israelian et al.(2001)/
/W.Aoki et al.(2006)/
/F.Primas et al.(2000)/
/E.Arnone et al.(2005)/
/P.E.Nissen et al.(2007)/
/C.J.Akerman et al.(2004)/
/G.Bihain et al.(2004)/
/J.Melendez et al.(2006)/
/P.E.Nissen et al.(2004)/
/A.Hosford et al.(2009)/
/C.Charbonnel and F. Primas(2005)/
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
/W.Aoki et al.(2009)/
/J.A.Rich and A. M. Boesgaard(2009)/
/M.Bergemann et al.(2010)/
/M.Ishigaki et al.(2010)/
/J.Melendez et al.(2010)/
/M.Bergemann and G. Cescutti(2010)/
/T.Gehren et al.(2006)/
/D.Fabbian et al.(2009)/
/C.J.Hansen et al.(2012)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/I.U.Roederer et al.(2014)/
/T.Matsuno et al.(2017)/
/D.S.Aguado et al.(2017)/
/T.Matsuno et al.(2017)/
/V.M.Placco et al.(2016)/
/A.M.Boesgaard et al.(2011)/
/I.U.Roederer et al.(2018)/
/A.M.Amarsi et al.(2019)/
/R.Smiljanic et al.(2021)/
/G.Israelian et al.(2004)/
Oxygen in the Very Early Galaxy
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 |
O I | N/A | -2.14 | 1.23 | ... | -1.85 | 1.52 | 6.84 | O I |
OH | N/A | -1.88+-0.31 | 1.49 | ... | -1.59+-0.31 | 1.78 | 7.10+-0.31 | OH |
Fe | N/A | -3.37+-0.16 | ... | ... | -3.37+-0.16 | ... | 4.13+-0.16 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-02-13 | N/A | VLT | 55000 | 120 | 20400 | N/A |
2000-02-15 | N/A | VLT | 55000 | 100 | 9600 | N/A |
HE 1327-2326, an Unevolved Star with [Fe/H]<-5.0. I. A Comprehensive Abundance Analysis
Stellar Parameters
Teff : 6390 | log g : 4.38 | vturb : 1.6 |
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 I | 1 | ... | ... | 2.30 | -0.96 | 2.29 | 2.30 | Li I |
CH | N/A | -2.71+-0.24 | +0.49+-0.24 | 5.68+-0.24 | -2.75+-0.24 | 0.50+-0.24 | 5.68+-0.24 | CH |
NH | N/A | -1.78+-0.30 | +1.42+-0.30 | 6.15+-0.30 | -1.68+-0.30 | 1.57+-0.30 | 6.15+-0.30 | NH |
OH | N/A | -2.32 | +0.88 | 6.34 | -2.35 | 0.90 | 6.34 | OH |
Na I | 1 | -4.23+-0.08 | -1.13+-0.08 | 2.10+-0.08 | -4.14+-0.08 | -0.89+-0.08 | 2.10+-0.08 | Na I |
Mg I | 5 | -2.74+-0.07 | +0.46+-0.07 | 4.80+-0.07 | -2.80+-0.07 | 0.45+-0.07 | 4.80+-0.07 | Mg I |
Al I | 1 | -3.72+-0.09 | -0.52+-0.09 | 2.75+-0.09 | -3.70+-0.09 | -0.45+-0.09 | 2.75+-0.09 | Al I |
Ca I | 6 | -2.74+-0.17 | +0.46+-0.17 | 3.62+-0.17 | -2.72+-0.17 | 0.53+-0.17 | 3.62+-0.17 | Ca I |
Ti II | 58 | -2.82+-0.20 | +0.38+-0.20 | 2.20+-0.20 | -2.75+-0.20 | 0.50+-0.20 | 2.20+-0.20 | Ti II |
Cr I | 3 | -3.38 | -0.18 | 2.26 | -3.38 | -0.13 | 2.26 | Cr I |
Mn I | 3 | -3.90 | -0.70 | 1.49 | -3.94 | -0.69 | 1.49 | Mn I |
Fe I | 59 | -3.20+-0.15 | ... | 4.25+-0.15 | -3.25+-0.15 | ... | 4.25+-0.15 | Fe I |
Fe II | 3 | -3.07 | +0.13 | 4.38 | -3.12 | +0.13 | 4.38 | Fe II |
Co I | 12 | -2.73 | +0.47 | 2.19 | -2.80 | 0.45 | 2.19 | Co I |
Ni I | 24 | -3.19 | +0.01 | 3.04 | -3.18 | 0.07 | 3.04 | Ni I |
Sr II | 2 | -3.02+-0.13 | +0.18+-0.13 | -0.10+-0.13 | -2.97+-0.13 | 0.28+-0.13 | -0.10+-0.13 | Sr II |
Ba II | 2 | -3.45 | -0.25 | -1.32 | -3.50 | -0.25 | -1.32 | Ba II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-06-02-9:52 | N/A | SUBARUHDS | 60000 | 20-260 | 20 | 443.84 |
2004-06-27-8:42 | N/A | SUBARUHDS | 60000 | 20-260 | 60 | 443.67 |
The beryllium abundance in the very metal-poor halo star G 64-12 from VLT/UVES observations
Stellar Parameters
Teff : 6400 | log g : 4.1 | 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 |
Li | N/A | ... | ... | 2.23+-0.01 | -1.03+-0.01 | 2.25+-0.01 | 2.23+-0.01 | Li |
Be | N/A | ... | ... | -1.05+-0.15 | -2.43+-0.15 | 0.85+-0.15 | -1.05+-0.15 | Be |
OH | N/A | ... | +1.1 | ... | -2.04 | 1.24 | 6.65 | OH |
Mg I | 2 | ... | +0.43+-0.03 | ... | -2.87+-0.03 | 0.41+-0.03 | 4.73+-0.03 | Mg I |
Ca I | 4 | ... | +0.48+-0.07 | ... | -2.78+-0.07 | 0.50+-0.07 | 3.56+-0.07 | Ca I |
Fe I | 22 | -3.28+-0.08 | ... | ... | -3.28+-0.08 | ... | 4.22+-0.08 | Fe I |
Fe II | 5 | -3.42+-0.10 | ... | ... | -3.42+-0.10 | ... | 4.08+-0.10 | Fe II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-02-12 | N/A | VLT | 48000 | 75-80 | 2x90min | N/A |
2000-02-12 | N/A | VLT | 55000 | 350-370 | 2x90min | N/A |
2000-02-14 | N/A | VLT | 48000 | 65-70 | 2x80min | N/A |
2000-02-14 | N/A | VLT | 55000 | 270-280 | 2x80min | N/A |
Mg abundances in metal-poor halo stars as a tracer of early Galactic mixing
Stellar Parameters
Teff : 6220 | log g : 3.9+-0.2 | vturb : 1.7+-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 |
Mg I | 3 | -3.08+-0.05 | 0.27+-0.05 | ... | -3.10+-0.05 | 0.25+-0.05 | 4.50+-0.05 | Mg I |
Ca I | 1 | -2.87 | ... | ... | -2.85 | 0.50 | 3.49 | Ca I |
Fe I | 4 | -3.35+-0.04 | ... | ... | -3.35+-0.04 | ... | 4.15+-0.04 | Fe I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | ANGLO | 40000 | >100 | N/A | N/A |
Sulphur and zinc abundances in Galactic halo stars revisited
Stellar Parameters
Teff : 6435 | log g : 4.26 | 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 | ... | 0.45 | ... | -2.58 | 0.66 | 4.54 | S I |
Fe | N/A | -3.24 | ... | ... | -3.24 | ... | 4.26 | Fe |
Zn I | N/A | ... | 0.41 | 1.77 | -2.79 | 0.45 | 1.77 | 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 |
The evolution of the C/O ratio in metal-poor halo stars
Stellar Parameters
Teff : 6511 | log g : 4.39 | 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 |
C I | N/A | ... | ... | 5.68 | -2.75 | 0.42 | 5.68 | C I |
O I | N/A | ... | ... | 6.44 | -2.25 | 0.92 | 6.44 | O I |
Fe | N/A | -3.17 | ... | ... | -3.17 | ... | 4.33 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 60000 | 200-300 | 3600 | N/A |
Cu and Zn in the early Galaxy
Stellar Parameters
Teff : 6318+-150 | log g : 4.20+-0.3 | vturb : 1.0 |
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 | -3.05 | ... | ... | -2.88 | ... | 4.62 | Fe |
Cu I | N/A | -4.00+-0.18 | ... | ... | -3.98+-0.18 | -1.10+-0.18 | 0.21+-0.18 | Cu I |
Zn I | N/A | <-2.35 | ... | ... | <-2.31 | <0.57 | <2.25 | Zn I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | VLT | 55000 | 80-150 | N/A | N/A |
PERMITTED OXYGEN ABUNDANCES AND THE TEMPERATURE SCALE OF METAL-POOR TURNOFF STARS
Stellar Parameters
Teff : 6660+-77 | log g : 4.24+-0.15 | 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 |
O I | N/A | ... | ... | 6.36 | -2.33 | 0.91 | 6.36 | O I |
Fe II | N/A | ... | ... | 4.26 | -3.24 | ... | 4.26 | Fe II |
Position
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 : 6511+-70 | log g : 4.39+-0.15 | vturb : 1.5+-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 | -2.81 | ... | ... | -2.73 | 0.44 | 4.39 | S I |
Fe II | N/A | -3.17 | ... | ... | -3.17 | ... | 4.33 | Fe II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001 | N/A | VLT | 60000 | 150-300 | N/A | N/A |
Lithium abundances of halo dwarfs based on excitation temperature. I. Local thermodynamic equilibrium
Stellar Parameters
Teff : 6333+-90 | log g : 4.49+-0.14 | 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 |
Li I | N/A | ... | ... | 2.21+-0.059 | -1.05+-0.059 | 2.27+-0.059 | 2.21+-0.059 | Li I |
Fe | N/A | -3.32 | ... | ... | -3.32 | ... | 4.18 | Fe |
Fe I | 59 | -3.40 | ... | ... | -3.40 | ... | 4.10 | Fe I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ANGLO | 43000 | 110 | N/A | N/A |
The lithium content of the 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 |
Li I | N/A | ... | ... | 2.347+0.074-0.089 | -0.91+0.074-0.089 | 2.47+0.074-0.089 | 2.347+0.074-0.089 | Li I |
Fe | N/A | -3.38+-0.130 | ... | ... | -3.38+-0.130 | ... | 4.12+-0.130 | Fe |
Lithium and Lithium Depletion in Halo Stars on Extreme Orbits
Stellar Parameters
Teff : 6074+-75 | log g : 3.72+-0.35 | vturb : 1.19+-0.48 |
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 I | N/A | ... | ... | 2.15+-0.06 | -1.11+-0.06 | 2.34+-0.06 | 2.15+-0.06 | Li I |
Fe | N/A | -3.47+-0.04 | ... | ... | -3.45+-0.04 | ... | 4.05+-0.04 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 48000 | 310 | N/A | N/A |
ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
Stellar Parameters
Teff : 6074+-75 | log g : 3.72+-0.35 | vturb : 1.19+-0.48 |
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 | -2.82+-0.16 | +0.63+-0.16 | ... | -2.84+-0.16 | 0.60+-0.16 | 4.76+-0.16 | Mg I |
Ca I | N/A | -2.84+-0.09 | +0.61+-0.10 | ... | -2.82+-0.09 | 0.62+-0.10 | 3.52+-0.09 | Ca I |
Ti | N/A | ... | +0.50+-0.11 | ... | -2.91+-0.11 | 0.53+-0.11 | 2.04+-0.11 | Ti |
Ti I | 1 | -2.92+-0.15 | ... | ... | -2.88+-0.15 | 0.56+-0.15 | 2.07+-0.15 | Ti I |
Ti II | 2 | -2.98+-0.13 | ... | ... | -2.94+-0.13 | 0.50+-0.13 | 2.01+-0.13 | Ti II |
Cr | N/A | ... | +0.07+-0.28 | ... | -3.35+-0.28 | 0.09+-0.28 | 2.29+-0.28 | Cr |
Cr I | 2 | -3.38+-0.28 | ... | ... | -3.35+-0.28 | 0.09+-0.28 | 2.29+-0.28 | Cr I |
Fe | N/A | -3.45+-0.04 | ... | ... | -3.44+-0.04 | ... | 4.06+-0.04 | Fe |
Fe I | 10 | -3.47+-0.05 | ... | ... | -3.46+-0.05 | ... | 4.04+-0.05 | Fe I |
Fe II | 3 | -3.40+-0.08 | ... | ... | -3.39+-0.08 | ... | 4.11+-0.08 | Fe II |
Ni I | N/A | -3.73+-0.16 | -0.28+-0.16 | ... | -3.70+-0.16 | -0.26+-0.16 | 2.52+-0.16 | Ni I |
Ba II | N/A | -3.65+-0.13 | -0.20+-0.14 | ... | -3.70+-0.13 | -0.26+-0.14 | -1.52+-0.13 | Ba II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2449904.241 | KECKHIRES | 48000 | 310 | 1200 | 442.6+-1.0 |
| 2449904.257 | KECKHIRES | 48000 | 310 | 1200 | 442.6+-1.0 |
LITHIUM ABUNDANCES OF EXTREMELY METAL-POOR TURNOFF STARS
Stellar Parameters
Teff : 6270+-100 | log g : 4.4 | 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 |
Li I | N/A | ... | ... | 2.18+-0.07 | -1.08+-0.07 | 2.34+-0.07 | 2.18+-0.07 | Li I |
Na I | N/A | ... | -0.06 | ... | -3.50 | -0.08 | 2.74 | Na I |
Mg I | N/A | ... | 0.37 | ... | -3.07 | 0.35 | 4.53 | Mg I |
Fe I | N/A | -3.37 | ... | ... | -3.42 | ... | 4.08 | Fe I |
Sr II | N/A | ... | 0.08 | ... | -3.24 | 0.18 | -0.37 | Sr II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-02-22 | 2453507.76 | SUBARUHDS | 90000 | N/A | 18000 | 434.68+-0.03 |
BERYLLIUM, OXYGEN, AND IRON ABUNDANCES IN EXTREMELY METAL-DEFICIENT 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 |
Be II | N/A | ... | ... | -1.43+-0.12 | -2.81+-0.12 | 0.64+-0.12 | -1.43+-0.12 | Be II |
OH | N/A | -2.24+-0.15 | ... | ... | -2.06+-0.15 | 1.39+-0.15 | 6.63+-0.15 | OH |
Fe | N/A | -3.45+-0.04 | ... | ... | -3.45+-0.04 | ... | 4.05+-0.04 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2005-05-15 | N/A | KECKHIRES | 48000 | 109 | 12600 | N/A |
NLTE analysis of Co i /Co ii lines in spectra of cool stars with new laboratory hyperfine splitting constants
Stellar Parameters
Teff : 6407+-80 | log g : 4.20+-0.20 | vturb : 2.3 |
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 | -3.12 | ... | ... | -3.12 | ... | 4.38 | Fe |
Co | 1 | ... | 0.19+-0.1 | ... | -2.93+-0.1 | 0.19+-0.1 | 2.06+-0.1 | Co |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | N/A | N/A | N/A | N/A |
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 6070+-70 | log g : 3.58 | vturb : 1.46 |
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 | -2.80+-0.03 | 0.76+-0.04 | ... | -2.82+-0.03 | 0.74+-0.04 | 4.78+-0.03 | Mg I |
Ca I | N/A | -3.05+-0.03 | 0.51+-0.03 | ... | -3.03+-0.03 | 0.53+-0.03 | 3.31+-0.03 | Ca I |
Ti | N/A | ... | 0.60+-0.04 | ... | -2.89+-0.04 | 0.67+-0.04 | 2.06+-0.04 | Ti |
Ti II | 2 | -2.96+-0.04 | ... | ... | -2.89+-0.04 | 0.67+-0.04 | 2.06+-0.04 | Ti II |
Cr | N/A | ... | -0.10+-0.04 | ... | -3.63+-0.04 | -0.07+-0.04 | 2.01+-0.04 | Cr |
Cr I | 1 | -3.66+-0.03 | ... | ... | -3.63+-0.03 | -0.07+-0.03 | 2.01+-0.03 | Cr I |
Fe I | 14 | -3.56+-0.01 | ... | ... | -3.56+-0.01 | ... | 3.94+-0.01 | Fe I |
Fe II | 2 | -3.56+-0.03 | ... | ... | -3.56+-0.03 | ... | 3.94+-0.03 | Fe II |
Ba II | N/A | -3.81+-0.04 | -0.25+-0.04 | ... | -3.86+-0.04 | -0.30+-0.04 | -1.68+-0.04 | Ba II |
Position
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 : 6463+-50 | log g : 4.17 |
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 | ... | ... | 2.32+-0.035 | -0.94+-0.035 | 2.32+-0.035 | 2.32+-0.035 | Li |
Fe | N/A | -3.26 | ... | ... | -3.26 | ... | 4.24 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | KECKHIRES | 85000 | >100 | N/A | N/A |
Chromium: NLTE abundances in metal-poor stars and nucleosynthesis in the Galaxy
Stellar Parameters
Teff : 6407+-100 | log g : 4.20+-0.05 | vturb : 2.3+-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 |
Cr I | 4 | ... | -0.26+-0.02 | ... | -3.36+-0.02 | -0.24+-0.02 | 2.28+-0.02 | Cr I |
Fe | N/A | -3.12 | ... | ... | -3.12 | ... | 4.38 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | N/A | N/A | N/A |
2001 | N/A | VLT | 40000 | N/A | N/A | N/A |
Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
Stellar Parameters
Teff : 6407 | log g : 4.20+-0.74 | vturb : 2.3 |
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 | 2 | ... | -0.24 | ... | -3.27 | -0.16 | 2.97 | Na I |
Mg I | 4 | ... | 0.14 | ... | -3.00 | 0.11 | 4.60 | Mg I |
Fe | N/A | -3.12 | ... | ... | -3.11 | ... | 4.39 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | 200 | 13850 | 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 | -2.72 | ... | 5.67 | -2.76 | 0.53 | 5.67 | C |
O | N/A | -2.21 | ... | 6.45 | -2.24 | 1.05 | 6.45 | O |
Fe | N/A | -3.24 | ... | ... | -3.29 | ... | 4.21 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001 | N/A | VLT | 60000 | N/A | N/A | N/A |
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
Teff : 6459+-100 | log g : 4.31+-0.25 | vturb : 1.5+-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 | -3.10+-0.15 | ... | ... | -3.10+-0.15 | ... | 4.40+-0.15 | Fe |
Sr | N/A | ... | -0.05+-0.10 | ... | -3.15+-0.10 | -0.05+-0.10 | -0.28+-0.10 | Sr |
Y | N/A | ... | 0.02+-0.13 | ... | -3.08+-0.13 | 0.02+-0.13 | -0.87+-0.13 | Y |
Ba | N/A | ... | -0.35+-0.16 | ... | -3.45+-0.16 | -0.35+-0.16 | -1.27+-0.16 | Ba |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 40000 | >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 : 6550+-100 | log g : 4.68+-0.3 | vturb : 1.90+-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 | ... | 0.32+-0.07 | ... | -2.89+-0.07 | 0.32+-0.07 | 4.71+-0.07 | Mg |
Ca | N/A | ... | 0.56+-0.06 | ... | -2.65+-0.06 | 0.56+-0.06 | 3.69+-0.06 | Ca |
Ti II | N/A | ... | 0.64+-0.10 | ... | -2.57+-0.10 | 0.64+-0.10 | 2.38+-0.10 | Ti II |
Fe I | N/A | -3.21+-0.08 | ... | ... | -3.21+-0.08 | ... | 4.29+-0.08 | Fe I |
Fe II | N/A | -3.22+-0.14 | ... | ... | -3.22+-0.14 | ... | 4.28+-0.14 | 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 | 430.5+-0.1 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 6550 | log g : 4.68 | 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 |
Sc II | N/A | ... | 0.37+-0.09 | ... | -2.87+-0.09 | 0.37+-0.09 | 0.28+-0.09 | Sc II |
Cr I | N/A | ... | -0.1+-0.07 | ... | -3.34+-0.07 | -0.10+-0.07 | 2.30+-0.07 | Cr I |
Fe I | N/A | -3.24+-0.09 | ... | ... | -3.24+-0.09 | ... | 4.26+-0.09 | Fe I |
Fe II | N/A | -3.22+-0.12 | ... | ... | -3.22+-0.12 | ... | 4.28+-0.12 | Fe II |
Ni I | N/A | ... | 0.12+-0.08 | ... | -3.12+-0.08 | 0.12+-0.08 | 3.10+-0.08 | Ni I |
Sr II | N/A | ... | 0.18+-0.12 | ... | -3.06+-0.12 | 0.18+-0.12 | -0.19+-0.12 | Sr II |
Ba II | N/A | ... | 0.06+-0.12 | ... | -3.18+-0.12 | 0.06+-0.12 | -1.00+-0.12 | Ba II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 90000 | N/A | N/A | N/A |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 6030+-36 | log g : 3.6+-0.18 | vturb : 1.2+-0.06 |
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 I | 1 | ... | ... | 2.08 | -1.18 | 2.40 | 2.08 | Li I |
CH | 1 | ... | <0.91 | <5.95 | <-2.48 | <1.10 | <5.95 | CH |
NH | 1 | ... | <2.16 | <6.60 | <-1.23 | <2.35 | <6.60 | NH |
O I | 3 | ... | <0.65 | <5.76 | <-2.93 | <0.65 | <5.76 | O I |
Na I | 1 | ... | -0.06+-0.22 | 2.60 | -3.64 | -0.06+-0.22 | 2.60 | Na I |
Mg I | 6 | ... | 0.50+-0.23 | 4.52 | -3.08 | 0.50+-0.23 | 4.52 | Mg I |
Al I | 2 | ... | -0.59+-0.21 | 2.28 | -4.17 | -0.59+-0.21 | 2.28 | Al I |
Si I | 1 | ... | 0.39+-0.32 | 4.32 | -3.19 | 0.39+-0.32 | 4.32 | Si I |
Ca I | 9 | ... | 0.62+-0.24 | 3.38 | -2.96 | 0.62+-0.24 | 3.38 | Ca I |
Sc II | 1 | ... | -0.24+-0.14 | -0.48 | -3.63 | -0.05+-0.14 | -0.48 | Sc II |
Ti I | 4 | ... | 0.70+-0.26 | 2.07 | -2.88 | 0.70+-0.26 | 2.07 | Ti I |
Ti II | 9 | ... | 0.11+-0.15 | 1.67 | -3.28 | 0.30+-0.15 | 1.67 | Ti II |
V II | 1 | ... | <0.82 | <1.36 | <-2.57 | <1.01 | <1.36 | V II |
Cr I | 3 | ... | -0.20+-0.21 | 1.85 | -3.79 | -0.21+-0.21 | 1.85 | Cr I |
Mn I | 1 | ... | -0.65+-0.27 | 1.20 | -4.23 | -0.65+-0.27 | 1.20 | Mn I |
Mn II | 1 | ... | -0.47+-0.25 | 1.57 | -3.86 | -0.28+-0.25 | 1.57 | Mn II |
Fe I | 39 | -3.58+-0.21 | ... | 3.92 | -3.58+-0.21 | ... | 3.92 | Fe I |
Fe II | 2 | -3.39+-0.16 | ... | 4.11 | -3.39+-0.16 | ... | 4.11 | Fe II |
Co I | 2 | ... | 0.34+-0.30 | 1.75 | -3.24 | 0.34+-0.30 | 1.75 | Co I |
Ni I | 4 | ... | 0.14+-0.26 | 2.77 | -3.45 | 0.13+-0.26 | 2.77 | Ni I |
Zn I | 2 | ... | <0.99 | <1.97 | <-2.59 | <0.99 | <1.97 | Zn I |
Rb I | 1 | ... | <3.54 | <2.48 | <0.12 | <3.70 | <2.48 | Rb I |
Sr II | 2 | ... | -0.10+-0.14 | -0.61 | -3.48 | 0.10+-0.14 | -0.61 | Sr II |
Y II | 6 | ... | <0.13 | <-1.05 | <-3.26 | <0.32 | <-1.05 | Y II |
Zr II | 3 | ... | <0.86 | <0.05 | <-2.53 | <1.05 | <0.05 | Zr II |
Nb II | 1 | ... | <3.27 | <1.34 | <-0.12 | <3.46 | <1.34 | Nb II |
Mo I | 1 | ... | <2.61 | <0.91 | <-0.97 | <2.61 | <0.91 | Mo I |
Tc I | 1 | ... | ... | <1.26 | <1.26 | <4.84 | <1.26 | Tc I |
Ba II | 1 | ... | -0.46+-0.16 | -1.67 | -3.85 | -0.27+-0.16 | -1.67 | Ba II |
Ce II | 5 | ... | <1.76 | <-0.05 | <-1.63 | <1.95 | <-0.05 | Ce II |
Pr II | 5 | ... | <2.12 | <-0.55 | <-1.27 | <2.31 | <-0.55 | Pr II |
Nd II | 5 | ... | <1.56 | <-0.41 | <-1.83 | <1.75 | <-0.41 | Nd II |
Sm II | 2 | ... | <2.18 | <-0.25 | <-1.21 | <2.37 | <-0.25 | Sm II |
Eu II | 4 | ... | <1.45 | <-1.42 | <-1.94 | <1.64 | <-1.42 | Eu II |
Gd II | 3 | ... | <2.36 | <0.04 | <-1.03 | <2.55 | <0.04 | Gd II |
Tb II | 4 | ... | <2.80 | <-0.29 | <-0.61 | <2.97 | <-0.29 | Tb II |
Dy II | 3 | ... | <1.82 | <-0.47 | <-1.57 | <2.01 | <-0.47 | Dy II |
Ho II | 1 | ... | <2.15 | <-0.76 | <-1.23 | <2.35 | <-0.76 | Ho II |
Er II | 3 | ... | <2.11 | <-0.36 | <-1.28 | <2.30 | <-0.36 | Er II |
Tm II | 2 | ... | <2.69 | <-0.60 | <-0.72 | <2.86 | <-0.60 | Tm II |
Yb II | 1 | ... | <1.30 | <-1.17 | <-2.09 | <1.49 | <-1.17 | Yb II |
Hf II | 2 | ... | <2.95 | <0.41 | <-0.30 | <3.28 | <0.41 | Hf II |
Pb I | 1 | ... | <3.00 | <1.46 | <-0.58 | <3.00 | <1.46 | Pb I |
Th II | 3 | ... | <2.67 | <-0.66 | <-0.72 | <2.86 | <-0.66 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | 442.7 |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2009-02-19-09:31 | 2454881.9 | MIKELCO | 41000 | 75-290 | 1200 | 442.7 |
High-resolution Spectroscopy of Extremely Metal-poor Stars from SDSS/SEGUE. III. Unevolved Stars with [Fe/H] ≲ -3.5
Stellar Parameters
Teff : 6285+-26 | log g : 4.30+-0.15 | vturb : 1.32+-0.18 |
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 I | 1 | ... | 5.60+-0.07 | 2.22+-0.07 | -1.04+-0.07 | 2.34+-0.07 | 2.22+-0.07 | Li I |
CH | 1 | ... | 0.92+-0.07 | 5.97+-0.07 | -2.46+-0.07 | 0.92+-0.07 | 5.97+-0.07 | CH |
Na I | 2 | ... | -0.07+-0.05 | 2.80+-0.06 | -3.44+-0.06 | -0.06+-0.05 | 2.80+-0.06 | Na I |
Mg I | 5 | ... | 0.37+-0.04 | 4.60+-0.05 | -3.00+-0.05 | 0.38+-0.04 | 4.60+-0.05 | Mg I |
Ca I | 15 | ... | 0.48+-0.02 | 3.44+-0.02 | -2.90+-0.02 | 0.48+-0.02 | 3.44+-0.02 | Ca I |
Sc II | 5 | ... | 0.21+-0.08 | -0.02+-0.07 | -3.17+-0.07 | 0.21+-0.08 | -0.02+-0.07 | Sc II |
Ti I | 6 | ... | 0.67+-0.03 | 2.25+-0.04 | -2.70+-0.04 | 0.68+-0.03 | 2.25+-0.04 | Ti I |
Ti II | 17 | ... | 0.53+-0.06 | 2.11+-0.06 | -2.84+-0.06 | 0.54+-0.06 | 2.11+-0.06 | Ti II |
Cr I | 6 | ... | -0.15+-0.02 | 2.11+-0.03 | -3.53+-0.03 | -0.15+-0.02 | 2.11+-0.03 | Cr I |
Fe I | 78 | ... | 0.00+-0.01 | 4.12+-0.02 | -3.38+-0.02 | 0.00+-0.01 | 4.12+-0.02 | Fe I |
Fe II | 15 | ... | 0.11+-0.07 | 4.23+-0.06 | -3.27+-0.06 | 0.11+-0.07 | 4.23+-0.06 | Fe II |
Sr II | 2 | ... | 0.18+-0.08 | -0.33+-0.08 | -3.20+-0.08 | 0.18+-0.08 | -0.33+-0.08 | Sr II |
Ba II | 2 | ... | -0.07+-0.07 | -1.27+-0.07 | -3.45+-0.07 | -0.07+-0.07 | -1.27+-0.07 | Ba II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-12-22 | N/A | SUBARUHDS | 90000 | 454-650 | N/A | N/A |
New ultra metal-poor stars from SDSS: follow-up GTC medium-resolution spectroscopy
Stellar Parameters
Position
Right Ascension : 13 40 02.4921790616 | Declination : -00 02 18.750321114 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
207-01-01 | N/A | OSIRISGTC | 2300 | 132 | 90 | N/A |
Lithium in CEMP-no stars: A new constraint on the lithium depletion mechanism in the early universe*
Stellar Parameters
Teff : 6291+-40 | log g : 4.38+-0.2 | vturb : 1.5+-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 I | N/A | ... | ... | 2.22+-0.06 | -1.04+-0.06 | 2.32+-0.06 | 2.22+-0.06 | Li I |
CH | N/A | ... | <0.93+-0.08 | ... | <-2.43+-0.08 | <0.93+-0.08 | <6.00+-0.08 | CH |
Na I | 2 | ... | -0.09+-0.05 | ... | -3.45+-0.05 | -0.09+-0.05 | 2.79+-0.05 | Na I |
Mg I | 5 | ... | 0.36+-0.03 | ... | -3.00+-0.03 | 0.36+-0.03 | 4.60+-0.03 | Mg I |
Ca I | 18 | ... | 0.51+-0.02 | ... | -2.85+-0.02 | 0.51+-0.02 | 3.49+-0.02 | Ca I |
Sc II | 4 | ... | 0.28+-0.09 | ... | -3.08+-0.09 | 0.28+-0.09 | 0.07+-0.09 | Sc II |
Ti I | 6 | ... | 0.66+-0.04 | ... | -2.70+-0.04 | 0.66+-0.04 | 2.25+-0.04 | Ti I |
Ti II | 18 | ... | 0.57+-0.07 | ... | -2.79+-0.07 | 0.57+-0.07 | 2.16+-0.07 | Ti II |
Cr I | 4 | ... | -0.11+-0.01 | ... | -3.47+-0.01 | -0.11+-0.01 | 2.17+-0.01 | Cr I |
Fe I | 49 | -3.36+-0.03 | ... | ... | -3.36+-0.03 | ... | 4.14+-0.03 | Fe I |
Fe II | 12 | ... | 0.11+-0.08 | ... | -3.25+-0.08 | 0.11+-0.08 | 4.25+-0.08 | Fe II |
Ba II | 2 | ... | -0.08+-0.08 | ... | -3.44+-0.08 | -0.08+-0.08 | -1.26+-0.08 | Ba II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 60000 | N/A | N/A | N/A |
G64-12 and G64-37 Are Carbon-enhanced Metal-poor Stars
Stellar Parameters
Teff : 6463+-50 | log g : 4.26+-0.15 | vturb : 1.65+-0.06 |
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 I | N/A | 1.31+-0.04 | 4.6+-0.04 | 2.36 | -0.90+-0.04 | 2.39+-0.04 | 2.36 | Li I |
CH | N/A | -2.22+-0.05 | 1.07+-0.05 | 6.21 | -2.22+-0.05 | 1.07+-0.05 | 6.21 | CH |
O I | N/A | -2.11+-0.07 | 1.18+-0.07 | 6.58 | -2.11+-0.07 | 1.18+-0.07 | 6.58 | O I |
Na I | N/A | -3.37+-0.03 | -0.08+-0.03 | 2.87 | -3.37+-0.03 | -0.08+-0.03 | 2.87 | Na I |
Mg I | N/A | -2.81+-0.07 | 0.48+-0.07 | 4.79 | -2.81+-0.07 | 0.48+-0.07 | 4.79 | Mg I |
Al I | N/A | -3.89+-0.05 | -0.6+-0.05 | 2.56 | -3.89+-0.05 | -0.60+-0.05 | 2.56 | Al I |
Si I | N/A | -3.45+-0.04 | -0.16+-0.04 | 4.06 | -3.45+-0.04 | -0.16+-0.04 | 4.06 | Si I |
Ca I | N/A | -2.78+-0.03 | 0.51+-0.03 | 3.56 | -2.78+-0.03 | 0.51+-0.03 | 3.56 | Ca I |
Sc II | N/A | -3.12+-0.06 | 0.17+-0.06 | 0.03 | -3.12+-0.06 | 0.17+-0.06 | 0.03 | Sc II |
Ti I | N/A | -2.55+-0.05 | 0.74+-0.05 | 2.4 | -2.55+-0.05 | 0.74+-0.05 | 2.4 | Ti I |
Ti II | N/A | -2.76+-0.09 | 0.53+-0.09 | 2.19 | -2.76+-0.09 | 0.53+-0.09 | 2.19 | Ti II |
Cr I | N/A | -3.37+-0.05 | -0.08+-0.05 | 2.27 | -3.37+-0.05 | -0.08+-0.05 | 2.27 | Cr I |
Mn I | N/A | -3.93+-0.05 | -0.64+-0.05 | 1.5 | -3.93+-0.05 | -0.64+-0.05 | 1.5 | Mn I |
Fe I | N/A | -3.29+-0.04 | ... | 4.21 | -3.29+-0.04 | ... | 4.21 | Fe I |
Fe II | N/A | -3.24+-0.06 | 0.05+-0.06 | 4.26 | -3.24+-0.06 | 0.05+-0.06 | 4.26 | Fe II |
Co I | N/A | -2.89+-0.05 | 0.4+-0.05 | 2.1 | -2.89+-0.05 | 0.40+-0.05 | 2.1 | Co I |
Ni I | N/A | -3.27+-0.03 | 0.02+-0.03 | 2.95 | -3.27+-0.03 | 0.02+-0.03 | 2.95 | Ni I |
Zn I | N/A | -2.76+-0.03 | 0.53+-0.03 | 1.8 | -2.76+-0.03 | 0.53+-0.03 | 1.8 | Zn I |
Sr II | N/A | -3.21+-0.06 | 0.08+-0.06 | -0.34 | -3.21+-0.06 | 0.08+-0.06 | -0.34 | Sr II |
Ba II | N/A | -3.35+-0.06 | -0.06+-0.06 | -1.17 | -3.35+-0.06 | -0.06+-0.06 | -1.17 | Ba II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 95000 | 700 | N/A | N/A |
Beryllium and Alpha-element Abundances in a Large Sample of Metal-poor Stars
Stellar Parameters
Teff : 6074+-100 | log g : 3.72+-0.2 | vturb : 1.5+-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 |
Be | N/A | ... | +0.60+-0.15 | -1.43+-0.12 | -2.81+-0.12 | 0.64+-0.15 | -1.43+-0.12 | Be |
O | N/A | -2.24+-0.22 | +1.21+-0.24 | ... | -2.30+-0.22 | 1.15+-0.24 | 6.39+-0.22 | O |
Mg | N/A | -2.76+-0.07 | ... | ... | -2.78+-0.07 | 0.67+-0.07 | 4.82+-0.07 | Mg |
Ti | N/A | -2.80+-0.09 | ... | ... | -2.73+-0.09 | 0.72+-0.09 | 2.22+-0.09 | Ti |
Fe | N/A | -3.45+-0.09 | ... | ... | -3.45+-0.09 | ... | 4.05+-0.09 | Fe |
Position
Right Ascension : | Declination : | 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 | KECKHIRES | 42000 | N/A | N/A | N/A |
Consistent Iron Abundances Derived from Neutral and Singly Ionized Iron Lines in Ultraviolet and Optical Spectra of Six Warm Metal-poor Stars
Stellar Parameters
Teff : 6492+-103 | log g : 4.18+-0.21 | vturb : 1.55+-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 |
Fe I | N/A | -3.26+-0.13 | ... | ... | -3.26+-0.13 | ... | 4.24+-0.13 | Fe I |
Fe II | N/A | -3.42+-0.10 | ... | ... | -3.42+-0.10 | ... | 4.08+-0.10 | Fe II |
Position
Right Ascension : | Declination : | 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 | HST | 30000 | 25 | N/A | N/A |
N/A | N/A | KECKHIRES | 49000 | 250 | N/A | N/A |
N/A | N/A | VLT | 41000 | 150 | N/A | N/A |
N/A | N/A | VLT | 42000 | 240 | N/A | N/A |
N/A | N/A | VLT | 42000 | 250 | 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 | ... | 0.44 | ... | -2.79 | 0.44 | 5.64 | C |
O | N/A | ... | 0.97 | ... | -2.26 | 0.97 | 6.43 | O |
Fe | N/A | -3.23 | ... | ... | -3.23 | ... | 4.27 | Fe |
Position
Right Ascension : 13 40 02.49 | Declination : -00 02 18.74 | 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 |
Inhomogeneity in the early Galactic chemical enrichment exposed by beryllium abundances in extremely metal-poor stars
Stellar Parameters
Teff : 6490+-145 | log g : 4.30+-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 |
Be | N/A | ... | ... | -13.1 | -14.48 | -11.22 | -13.1 | Be |
Fe | N/A | -3.26+-0.03 | ... | ... | -3.26+-0.03 | ... | 4.24+-0.03 | Fe |
Position
Right Ascension : 13 40 02.50 | Declination : -00 02 18.84 | 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 | N/A | 120 | N/A | N/A |
Galactic evolution of nitrogen
Stellar Parameters
Teff : 6318+-150 | log g : 4.20+-0.30 | vturb : 1.00 |
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 |
NH | N/A | -1.90+-0.25 | ... | ... | -1.68+-0.25 | 1.20+-0.25 | 6.15+-0.25 | NH |
Fe | N/A | -3.05 | ... | ... | -2.88 | ... | 4.62 | Fe |
Position
Right Ascension : | Declination : | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-02-13 | N/A | VLT | 55000 | 120 | 20400 | N/A |
2000-02-15 | N/A | VLT | 55000 | 100 | 9600 | N/A |