HD37828
taken from 5 paper(s):
/J.Melendez and B. Barbuy(2001)/
/T.V.Mishenina et al.(2002)/
/T.V.Mishenina and V. V. Kovtyukh(2001)/
/J.Simmerer et al.(2004)/
/I.U.Roederer et al.(2010)/
Oxygen Abundances in Metal-poor Stars (-2.2 < [Fe/H] < -1.2) from Infrared OH Lines
Stellar Parameters
Teff : 4326 | log g : 1.05 | vturb : 1.3 |
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 |
O | N/A | -0.88 | 0.54 | ... | -0.70 | 0.72 | 7.99 | O |
Fe | N/A | -1.42 | ... | ... | -1.42 | ... | 6.08 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1999-09-21 | N/A | PHOENIXKPNO | 60000 | 105 | 2x300 | N/A |
1999-09-26 | N/A | PHOENIXKPNO | 60000 | 105 | 2x300 | N/A |
1999-09-27 | N/A | PHOENIXKPNO | 50000 | 100 | 2x300 | N/A |
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 | -1.49 | ... | ... | -1.49 | ... | 6.01 | Fe |
Cu I | N/A | ... | -0.41+-0.25 | ... | -1.88+-0.25 | -0.39+-0.25 | 2.31+-0.25 | Cu I |
Zn I | N/A | ... | 0.04+-0.26 | ... | -1.41+-0.26 | 0.08+-0.26 | 3.15+-0.26 | 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 : 4350 | log g : 1.0 | 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 |
Mg I | N/A | ... | 0.26 | ... | -1.34 | 0.24 | 6.26 | Mg I |
Si I | N/A | ... | 0.42 | ... | -1.12 | 0.46 | 6.39 | Si I |
Ca I | N/A | ... | 0.47 | ... | -1.09 | 0.49 | 5.25 | Ca I |
Fe | N/A | -1.58 | ... | ... | -1.58 | ... | 5.92 | Fe |
Sr I | N/A | ... | 0.01 | ... | -1.47 | 0.11 | 1.40 | Sr I |
Ba II | N/A | ... | 0.08 | ... | -1.55 | 0.03 | 0.63 | Ba II |
La II | N/A | ... | 0.18 | ... | -1.33 | 0.25 | -0.23 | La II |
Ce II | N/A | ... | 0.17 | ... | -1.41 | 0.17 | 0.17 | Ce II |
Nd II | N/A | ... | 0.39 | ... | -1.11 | 0.47 | 0.31 | Nd II |
Eu II | N/A | ... | 0.35 | ... | -1.24 | 0.34 | -0.72 | 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
Stellar Parameters
Teff : 4350 | log g : 1.50 | vturb : 1.85 |
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 | ... | -0.2 | ... | -1.64 | -0.02 | 6.79 | C |
Fe I | 17 | -1.62 | ... | ... | -1.62 | ... | 5.88 | Fe I |
Fe II | 9 | -1.42 | ... | ... | -1.42 | ... | 6.08 | Fe II |
La II | N/A | ... | ... | -0.12+-0.06 | -1.22+-0.06 | 0.40+-0.06 | -0.12+-0.06 | La II |
Eu II | N/A | ... | ... | -0.53+-0.04 | -1.05+-0.04 | 0.57+-0.04 | -0.53+-0.04 | 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 |
THE UBIQUITY OF THE RAPID NEUTRON-CAPTURE PROCESS
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 | -1.62 | ... | ... | -1.62 | ... | 5.88 | Fe |
Zn I | N/A | ... | ... | 3.18 | -1.38 | 0.24 | 3.18 | Zn I |
Y II | N/A | ... | ... | 0.7 | -1.51 | 0.11 | 0.7 | Y II |
Pb I | N/A | ... | ... | 0.77 | -1.27 | 0.35 | 0.77 | Pb I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |