HD150177
taken from 2 paper(s):
/T.V.Mishenina et al.(2002)/
/T.V.Mishenina and V. V. Kovtyukh(2001)/
T.V.Mishenina et al.,AAP, 396, 189, 2002 (A0070,ADS)
Abundances of Cu and Zn in metal-poor stars: Clues for Galaxy evolution
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 | -0.65 | ... | ... | -0.65 | ... | 6.85 | Fe |
| Cu I | N/A | ... | -0.15+-0.12 | ... | -0.78+-0.12 | -0.13+-0.12 | 3.41+-0.12 | Cu I |
| Zn I | N/A | ... | 0.01+-0.11 | ... | -0.60+-0.11 | 0.05+-0.11 | 3.96+-0.11 | Zn I |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| N/A | N/A | ELODIE | 42000 | >100 | N/A | N/A |
| Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
T.V.Mishenina et al.,AAP, 370, 951, 2001 (A0071,ADS)
Analysis of neutron capture elements in metal-poor stars
Stellar Parameters
| Teff : 6025 | log g : 3.8 | vturb : 1.1 |
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 | ... | 0.05 | ... | -0.61 | 0.03 | 6.99 | Mg I |
| Si I | N/A | ... | 0.13 | ... | -0.47 | 0.17 | 7.04 | Si I |
| Ca I | N/A | ... | 0.17 | ... | -0.45 | 0.19 | 5.89 | Ca I |
| Fe | N/A | -0.64 | ... | ... | -0.64 | ... | 6.86 | Fe |
| Ba II | N/A | ... | 0.28 | ... | -0.41 | 0.23 | 1.77 | Ba II |
| La II | N/A | ... | -0.12 | ... | -0.69 | -0.05 | 0.41 | La II |
| Ce II | N/A | ... | -0.05 | ... | -0.69 | -0.05 | 0.89 | Ce II |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| N/A | N/A | ELODIE | 42000 | >100 | N/A | N/A |