HD104800
/T.Gehren et al.(2006)/ /B.E.Reddy et al.(2006)/
Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
Right Ascension : 12 04 05.56 | Declination : +03 20 26.7 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
N/A | FOCES | 40000 | 200 | 5400 | N/A |
Elemental abundance survey of the Galactic thick disc
Teff : 5663 | log g : 4.63 |
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 | ... | 0.28 | ... | -0.43 | 0.41 | 8.00 | C |
Na | N/A | ... | 0.05 | ... | -0.71 | 0.13 | 5.53 | Na |
Mg | N/A | ... | 0.28 | ... | -0.57 | 0.27 | 7.03 | Mg |
Al | N/A | ... | 0.22 | ... | -0.74 | 0.10 | 5.71 | Al |
Si | N/A | ... | 0.23 | ... | -0.45 | 0.39 | 7.06 | Si |
Ca | N/A | ... | 0.21 | ... | -0.59 | 0.25 | 5.75 | Ca |
Sc | N/A | ... | 0.05 | ... | -0.65 | 0.19 | 2.50 | Sc |
Ti | N/A | ... | 0.22 | ... | -0.62 | 0.22 | 4.33 | Ti |
V | N/A | ... | 0.05 | ... | -0.67 | 0.17 | 3.26 | V |
Mn | N/A | ... | -0.33 | ... | -1.18 | -0.34 | 4.25 | Mn |
Fe I | N/A | -0.79 | ... | ... | -0.84 | ... | 6.66 | Fe I |
Co | N/A | ... | 0.13 | ... | -0.72 | 0.12 | 4.27 | Co |
Ni | N/A | ... | 0.03 | ... | -0.75 | 0.09 | 5.47 | Ni |
Cu | N/A | ... | -0.03 | ... | -0.82 | 0.02 | 3.37 | Cu |
Zn | N/A | ... | 0.09 | ... | -0.79 | 0.05 | 3.77 | Zn |
Y | N/A | ... | 0.18 | ... | -0.70 | 0.14 | 1.51 | Y |
Ce | N/A | ... | 0.08 | ... | -0.71 | 0.13 | 0.87 | Ce |
Nd | N/A | ... | 0.09 | ... | -0.62 | 0.22 | 0.80 | Nd |
Eu | N/A | ... | 0.44 | ... | -0.26 | 0.58 | 0.26 | Eu |
Vrad | 6.8 |
Right Ascension : 12 04 05.56 | Declination : +03 20 26.7 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2004-06 | N/A | MCDONALD | 60000 | 100-200 | N/A | 6.8 |