SDSSJ1742+2531
TOPoS . II. On the bimodality of carbon abundance in CEMP stars Implications on the early chemical evolution of galaxies
Teff : 6345 | log g : 4.0 | vturb : 1.5 |
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 | ... | ... | 7.26 | -1.17 | 3.63 | 7.26 | C |
CH | N/A | ... | ... | 7.26 | -1.17 | 3.63 | 7.26 | CH |
O I | N/A | ... | ... | <6.92 | <-1.77 | <3.03 | <6.92 | O I |
Na I | N/A | ... | ... | <2.14 | <-4.10 | <0.70 | <2.14 | Na I |
Mg I | N/A | ... | ... | <3.07 | <-4.53 | <0.27 | <3.07 | Mg I |
Si I | N/A | ... | ... | <3.05 | <-4.46 | <0.34 | <3.05 | Si I |
S I | N/A | ... | ... | <4.61 | <-2.51 | <2.29 | <4.61 | S I |
Ca | N/A | -4.56 | ... | ... | -4.54 | 0.26 | 1.80 | Ca |
Ca I | N/A | ... | ... | <1.62 | <-4.72 | <0.08 | <1.62 | Ca I |
Ca II | N/A | ... | ... | 1.79+-0.04 | -4.55+-0.04 | 0.25+-0.04 | 1.79+-0.04 | Ca II |
Fe | N/A | -4.80 | ... | ... | -4.80 | ... | 2.70 | Fe |
Fe I | N/A | ... | ... | 2.73+-0.09 | -4.77+-0.09 | ... | 2.73+-0.09 | Fe I |
Sr II | N/A | ... | ... | <-1.25+-2.92 | <-4.12+-2.92 | <0.68+-2.92 | <-1.25+-2.92 | Sr II |
Ba II | N/A | ... | ... | <-0.97+-2.17 | <-3.15+-2.17 | <1.65+-2.17 | <-0.97+-2.17 | Ba II |
Vrad | -207.5+-0.5 |
Right Ascension : 17 42 59.68 | Declination : +25 31 35.9 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2013-04-17 | N/A | VLT | 47000 | 3-45 | 84000 | -207.5+-0.5 |