HE1410+0213
taken from 3 paper(s):
/J.G.Cohen et al.(2006)/
/J.G.Cohen et al.(2013)/
/T.Masseron et al.(2010)/
Carbon Stars in the Hamburg/ESO Survey: Abundances
Stellar Parameters
| Teff : 4985 | log g : 2.0 | vturb : 1.8 |
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 |
|---|
| CH | 1 | ... | 1.73 | 8.16 | -0.27 | 1.94 | 8.16 | CH |
| CN | 1 | ... | 1.78 | 7.55 | -0.28 | 1.93 | 7.55 | CN |
| Mg I | 2 | ... | 0.18+-0.03 | 5.56+-0.03 | -2.04+-0.03 | 0.17+-0.03 | 5.56+-0.03 | Mg I |
| Ti I | 2 | ... | 0.29+-0.04 | 3.12+-0.04 | -1.83+-0.04 | 0.38+-0.04 | 3.12+-0.04 | Ti I |
| Ti II | 1 | ... | 0.36 | 3.19 | -1.76 | 0.45 | 3.19 | Ti II |
| Cr I | 1 | ... | -0.55 | 2.96 | -2.68 | -0.47 | 2.96 | Cr I |
| Fe I | 12 | -2.16+-0.31 | ... | 5.29+-0.31 | -2.21+-0.31 | ... | 5.29+-0.31 | Fe I |
| Fe II | 3 | ... | -0.41+-0.21 | 4.88+-0.21 | -2.62+-0.21 | -0.41+-0.21 | 4.88+-0.21 | Fe II |
| Ba II | 1 | ... | 0.07 | 0.04 | -2.14 | 0.07 | 0.04 | Ba II |
Position
| Right Ascension : 14 13 06.50 | Declination : +01 59 21.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| N/A | KECKHIRES | 45000 | 80 | 2700 | N/A |
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
Stellar Parameters
| Teff : 5000+-100 | log g : 2+-0.25 | vturb : 1.8+-0.2 |
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 |
|---|
| CH | N/A | ... | 1.71 | ... | -0.27 | 1.92 | 8.16 | CH |
| NH | 1 | ... | 1.76 | ... | -0.28 | 1.91 | 7.55 | NH |
| Mg I | 2 | ... | 0.16+-0.02 | ... | -2.04+-0.02 | 0.15+-0.02 | 5.56+-0.02 | Mg I |
| Ti I | 2 | ... | 0.24+-0.04 | ... | -1.86+-0.04 | 0.33+-0.04 | 3.09+-0.04 | Ti I |
| Ti II | 1 | ... | 0.38 | ... | -1.72 | 0.47 | 3.23 | Ti II |
| Cr I | 1 | ... | -0.65 | ... | -2.76 | -0.57 | 2.88 | Cr I |
| Fe I | N/A | -2.14+-0.33 | ... | ... | -2.19+-0.33 | ... | 5.31+-0.33 | Fe I |
| Fe II | 4 | -2.4+-0.35 | -0.26+-0.35 | ... | -2.45+-0.35 | -0.26+-0.35 | 5.05+-0.35 | Fe II |
| Ba II | 1 | ... | -0.26 | ... | -2.45 | -0.26 | -0.27 | Ba II |
Binary Parameters
Position
| Right Ascension : 14 13 06.50 | Declination : +01 59 21.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2002-05 | N/A | KECKHIRES | 36000 | 135 | 2700 | 80.7 |
A holistic approach to carbon-enhanced metal-poor stars
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 |
|---|
| C | N/A | ... | 2.33+-0.1 | ... | -0.23+-0.1 | 2.34+-0.1 | 8.20+-0.1 | C |
| N | N/A | ... | 2.94+-0.1 | ... | 0.37+-0.1 | 2.94+-0.1 | 8.20+-0.1 | N |
| O | N/A | ... | 2.56+-0.2 | ... | 0.01+-0.2 | 2.58+-0.2 | 8.70+-0.2 | O |
| Mg | N/A | ... | 0.33+-0.18 | ... | -2.26+-0.18 | 0.31+-0.18 | 5.34+-0.18 | Mg |
| Fe | N/A | -2.52+-0.21 | ... | ... | -2.57+-0.21 | ... | 4.93+-0.21 | Fe |
| Ba | N/A | ... | 0.05+-0.2 | ... | -2.48+-0.2 | 0.09+-0.2 | -0.30+-0.2 | Ba |
| La | N/A | ... | 0.41+-0.2 | ... | -2.08+-0.2 | 0.49+-0.2 | -0.98+-0.2 | La |
| Ce | N/A | ... | 0.85+-0.3 | ... | -1.67+-0.3 | 0.90+-0.3 | -0.09+-0.3 | Ce |
| Eu | N/A | ... | <0.91 | ... | <-1.61 | <0.96 | <-1.09 | Eu |
| Pb | N/A | ... | <1.33 | ... | <-1.21 | <1.36 | <0.83 | Pb |
Isotopic Ratio
Position
| Right Ascension : 14 13 06.50 | Declination : +01 59 21.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| N/A | N/A | R=40000 | N/A | N/A | N/A |