HD5750
/K.A.Venn et al.(2004)/ /Y.Q.Chen et al.(2000)/
Stellar Chemical Signatures and Hierarchical Galaxy Formation
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 | ... | 0.08 | ... | -0.22 | 0.17 | 6.02 | Na |
Mg | N/A | ... | 0.01 | ... | -0.40 | -0.01 | 7.20 | Mg |
Ca | N/A | ... | 0.07 | ... | -0.30 | 0.09 | 6.04 | Ca |
Ti | N/A | ... | 0.06 | ... | -0.26 | 0.13 | 4.69 | Ti |
Fe | N/A | -0.39 | ... | ... | -0.39 | ... | 7.11 | Fe |
Ni | N/A | ... | -0.05 | ... | -0.41 | -0.02 | 5.81 | Ni |
Y | N/A | ... | -0.18 | ... | -0.54 | -0.15 | 1.67 | Y |
Ba | N/A | ... | -0.06 | ... | -0.50 | -0.11 | 1.68 | Ba |
Right Ascension : 00 59 35.80 | Declination : +32 29 32.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Chemical composition of 90 F and G disk dwarfs
Teff : 6223+-70 | log g : 4.21+-0.1 | vturb : 1.93+-0.3 |
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 | ... | 0.14 | ... | -0.12 | 0.32 | 8.57 | O |
Na | N/A | ... | -0.05 | ... | -0.40 | 0.04 | 5.84 | Na |
Mg | N/A | ... | 0.25 | ... | -0.21 | 0.23 | 7.39 | Mg |
Si | N/A | ... | 0.07 | ... | -0.33 | 0.11 | 7.18 | Si |
K | N/A | ... | 0.26 | ... | -0.09 | 0.35 | 4.94 | K |
Ca | N/A | ... | 0.08 | ... | -0.34 | 0.10 | 6.00 | Ca |
Cr | N/A | ... | -0.05 | ... | -0.46 | -0.02 | 5.18 | Cr |
Fe I | N/A | -0.44 | ... | ... | -0.44 | ... | 7.06 | Fe I |
Fe II | N/A | -0.4 | ... | ... | -0.40 | ... | 7.10 | Fe II |
Ni | N/A | ... | -0.03 | ... | -0.44 | 0.00 | 5.78 | Ni |
Ba | N/A | ... | 0.17 | ... | -0.32 | 0.12 | 1.86 | Ba |
Right Ascension : 00 59 35.80 | Declination : +32 29 32.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
1997-03-21 | N/A | CESESO | 40000 | 200-400 | N/A | N/A |