HR219
taken from 2 paper(s):
/J.Simmerer et al.(2004)/
/K.A.Venn et al.(2004)/
J.Simmerer et al.,ApJ, 617, 1091, 2004 (A0131,ADS)
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 | -0.36 | ... | ... | -0.36 | ... | 7.14 | Fe I |
| Fe II | N/A | -0.44 | ... | ... | -0.44 | ... | 7.06 | Fe II |
| La II | N/A | ... | ... | 0.82 | -0.28 | 0.08 | 0.82 | La II |
| Eu II | N/A | ... | ... | 0.15 | -0.37 | -0.01 | 0.15 | Eu II |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
| Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
K.A.Venn et al.,AJ, 128, 1177, 2004 (C0011,ADS)
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 | ... | 0.01 | ... | -0.21 | 0.10 | 6.03 | Na |
| Mg | N/A | ... | 0.16 | ... | -0.17 | 0.14 | 7.43 | Mg |
| Ca | N/A | ... | 0.06 | ... | -0.23 | 0.08 | 6.11 | Ca |
| Ti | N/A | ... | 0.11 | ... | -0.13 | 0.18 | 4.82 | Ti |
| Fe | N/A | -0.31 | ... | ... | -0.31 | ... | 7.19 | Fe |
| Ni | N/A | ... | 0.03 | ... | -0.25 | 0.06 | 5.97 | Ni |
| Y | N/A | ... | -0.01 | ... | -0.29 | 0.02 | 1.92 | Y |
| Ba | N/A | ... | -0.17 | ... | -0.53 | -0.22 | 1.65 | Ba |
Observing Log
| Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : +574855 | Right Ascension : 004906.3 |