HR3775
taken from 3 paper(s):
/J.Simmerer et al.(2004)/
/A.M.Boesgaard et al.(1999)/
/K.A.Venn et al.(2004)/
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 | -0.22 | ... | ... | -0.22 | ... | 7.28 | Fe I |
Fe II | N/A | -0.28 | ... | ... | -0.28 | ... | 7.22 | Fe II |
La II | N/A | ... | ... | 0.98 | -0.12 | 0.10 | 0.98 | La II |
Eu II | N/A | ... | ... | 0.36 | -0.16 | 0.06 | 0.36 | 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 |
OXYGEN IN UNEVOLVED METAL-POOR STARS FROM KECK ULTRAVIOLET HIRES SPECTRA
Stellar Parameters
Teff : 6300 | log g : 4.10 | 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 | N/A | -0.01+-0.10 | 0.16+-0.14 | 8.92 | 0.23+-0.10 | 0.23+-0.14 | 8.92 | O |
Fe | N/A | -0.17 | ... | ... | 0.00 | ... | 7.50 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1994-03-01 | N/A | KECKHIRES | 45000 | 95 | 180 | 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 | ... | 0.03 | ... | -0.08 | 0.12 | 6.16 | Na |
Mg | N/A | ... | 0.09 | ... | -0.13 | 0.07 | 7.47 | Mg |
Ca | N/A | ... | 0.07 | ... | -0.11 | 0.09 | 6.23 | Ca |
Ti | N/A | ... | 0.08 | ... | -0.05 | 0.15 | 4.90 | Ti |
Fe | N/A | -0.2 | ... | ... | -0.20 | ... | 7.30 | Fe |
Ni | N/A | ... | 0.02 | ... | -0.15 | 0.05 | 6.07 | Ni |
Y | N/A | ... | 0.25 | ... | 0.08 | 0.28 | 2.29 | Y |
Ba | N/A | ... | 0.08 | ... | -0.17 | 0.03 | 2.01 | Ba |