HD18768
taken from 5 paper(s):
/T.V.Mishenina et al.(2002)/
/T.V.Mishenina and V. V. Kovtyukh(2001)/
/J.Simmerer et al.(2004)/
/M.Takada-Hidai et al.(2002)/
/K.A.Venn et al.(2004)/
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 | -0.51 | ... | ... | -0.51 | ... | 6.99 | Fe |
Cu I | N/A | ... | -0.12+-0.25 | ... | -0.61+-0.25 | -0.10+-0.25 | 3.58+-0.25 | Cu I |
Zn I | N/A | ... | 0.21+-0.23 | ... | -0.26+-0.23 | 0.25+-0.23 | 4.30+-0.23 | Zn I |
Position
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 : 5700 | log g : 3.5 | 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 |
Mg I | N/A | ... | 0.00 | ... | -0.53 | -0.02 | 7.07 | Mg I |
Si I | N/A | ... | 0.10 | ... | -0.37 | 0.14 | 7.14 | Si I |
Ca I | N/A | ... | 0.15 | ... | -0.34 | 0.17 | 6.00 | Ca I |
Fe | N/A | -0.51 | ... | ... | -0.51 | ... | 6.99 | Fe |
Sr I | N/A | ... | -0.04 | ... | -0.45 | 0.06 | 2.42 | Sr I |
Ba II | N/A | ... | 0.22 | ... | -0.34 | 0.17 | 1.84 | Ba II |
La II | N/A | ... | 0.03 | ... | -0.41 | 0.10 | 0.69 | La II |
Ce II | N/A | ... | -0.06 | ... | -0.57 | -0.06 | 1.01 | Ce II |
Nd II | N/A | ... | 0.01 | ... | -0.42 | 0.09 | 1.00 | Nd II |
Eu II | N/A | ... | 0.26 | ... | -0.26 | 0.25 | 0.26 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ELODIE | 42000 | >100 | N/A | N/A |
The Rise of the s-Process in the Galaxy
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 | -0.65 | ... | ... | -0.65 | ... | 6.85 | Fe I |
Fe II | N/A | -0.71 | ... | ... | -0.71 | ... | 6.79 | Fe II |
La II | N/A | ... | ... | 0.45 | -0.65 | 0.00 | 0.45 | La II |
Eu II | N/A | ... | ... | -0.07 | -0.59 | 0.06 | -0.07 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Behavior of Sulfur Abundances in Metal-poor Giants and Dwarfs
Stellar Parameters
Teff : 5750+-100 | log g : 3.84+-0.15 | vturb : 1.9+-0.5 |
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 | -0.36 | ... | 6.86 | -0.26 | 0.53 | 6.86 | S I |
Fe I | N/A | -0.70 | ... | 6.71 | -0.79 | ... | 6.71 | Fe I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | OAO | 24500 | 120-400 | N/A | N/A |
Stellar Chemical Signatures and Hierarchical Galaxy Formation
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 | ... | 0.1 | ... | -0.43 | 0.19 | 5.81 | Na |
Mg | N/A | ... | 0.17 | ... | -0.47 | 0.15 | 7.13 | Mg |
Ca | N/A | ... | 0.05 | ... | -0.55 | 0.07 | 5.79 | Ca |
Ti | N/A | ... | 0.09 | ... | -0.46 | 0.16 | 4.49 | Ti |
Fe | N/A | -0.62 | ... | ... | -0.62 | ... | 6.88 | Fe |
Ni | N/A | ... | 0.04 | ... | -0.55 | 0.07 | 5.67 | Ni |
Y | N/A | ... | -0.11 | ... | -0.70 | -0.08 | 1.51 | Y |
Ba | N/A | ... | -0.25 | ... | -0.92 | -0.30 | 1.26 | Ba |