CS22174-007
taken from 3 paper(s):
/J.A.Johnson et al.(2007)/
/W.Aoki et al.(2007)/
/D.M.Allen et al.(2012)/
A Search for Nitrogen-enhanced Metal-poor Stars
Stellar Parameters
Teff : 5059 | log g : 2.37 | vturb : 1.69 |
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 | ... | -0.40+-0.29 | 6.16+-0.25 | -2.27+-0.25 | -0.29+-0.29 | 6.16+-0.25 | C |
N | N/A | ... | <-0.89+-0.25 | <5.16+-0.25 | <-2.67+-0.25 | <-0.69+-0.25 | <5.16+-0.25 | N |
Fe | N/A | -2.00+-0.21 | ... | ... | -1.98+-0.21 | ... | 5.52+-0.21 | Fe |
Position
Right Ascension : 01 14 06.48 | Declination : -11 02 35.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-08-30 | N/A | RCCTIO | N/A | 142 | 5400 | N/A |
Carbon-enhanced Metal-poor Stars. I. Chemical Compositions of 26 Stars
Stellar Parameters
Teff : 5300 | log g : 2.7 | vturb : 2.1 |
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 | ... | 0.41+-0.16 | 6.6+-0.16 | -1.83+-0.16 | 0.41+-0.16 | 6.6+-0.16 | C |
CN | N/A | ... | <1.42+-0.07 | <7.0+-0.07 | <-0.83+-0.07 | <1.41+-0.07 | <7.0+-0.07 | CN |
Na I | 2 | ... | 0.30+-0.17 | 4.27+-0.17 | -1.97+-0.17 | 0.27+-0.17 | 4.27+-0.17 | Na I |
Mg I | 5 | ... | 0.49+-0.10 | 5.82+-0.10 | -1.78+-0.10 | 0.46+-0.10 | 5.82+-0.10 | Mg I |
Ca I | 10 | ... | 0.24+-0.10 | 4.35+-0.10 | -1.99+-0.10 | 0.25+-0.10 | 4.35+-0.10 | Ca I |
Sc II | 3 | ... | 0.11+-0.14 | 0.96+-0.14 | -2.19+-0.14 | 0.05+-0.14 | 0.96+-0.14 | Sc II |
Ti I | 8 | ... | 0.39+-0.09 | 3.09+-0.09 | -1.86+-0.09 | 0.38+-0.09 | 3.09+-0.09 | Ti I |
Ti II | 22 | ... | 0.46+-0.14 | 3.17+-0.14 | -1.78+-0.14 | 0.46+-0.14 | 3.17+-0.14 | Ti II |
Cr I | 7 | ... | -0.19+-0.09 | 3.26+-0.09 | -2.38+-0.09 | -0.14+-0.09 | 3.26+-0.09 | Cr I |
Fe I | 85 | -2.20+-0.14 | ... | 5.26+-0.14 | -2.24+-0.14 | ... | 5.26+-0.14 | Fe I |
Fe II | 12 | -2.20+-0.13 | ... | 5.26+-0.13 | -2.24+-0.13 | ... | 5.26+-0.13 | Fe II |
Ni I | 2 | ... | 0.03+-0.11 | 4.07+-0.11 | -2.15+-0.11 | 0.09+-0.11 | 4.07+-0.11 | Ni I |
Zn I | 2 | ... | 0.06+-0.13 | 2.46+-0.13 | -2.10+-0.13 | 0.14+-0.13 | 2.46+-0.13 | Zn I |
Ba II | 4 | ... | -0.57+-0.13 | -0.59+-0.13 | -2.77+-0.13 | -0.53+-0.13 | -0.59+-0.13 | Ba II |
Binary Parameters
Position
Right Ascension : 01 14 06.48 | Declination : -11 02 35.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-10-26 | N/A | SUBARUHDS | 50000 | N/A | 600 | -70.76+-0.03 |
Elemental abundances and classification of carbon-enhanced metal-poor stars
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 | -2.46 | 0.25 | ... | -2.37 | 0.25 | 6.06 | C |
N | N/A | <-2.11 | <0.60 | ... | <-1.97 | <0.60 | <5.86 | N |
Ti I | N/A | -2.43 | 0.28 | ... | -2.36 | 0.28 | 2.59 | Ti I |
Ti II | N/A | -2.33 | 0.38 | ... | -2.26 | 0.38 | 2.69 | Ti II |
Zn | N/A | -2.56 | 0.15 | ... | -2.52 | 0.15 | 2.04 | Zn |
Sr | N/A | -2.93 | -0.22 | ... | -2.83 | -0.22 | 0.04 | Sr |
Y | N/A | -3.02 | -0.31 | ... | -2.99 | -0.31 | -0.78 | Y |
Zr | N/A | -2.67 | 0.04 | ... | -2.65 | 0.04 | -0.07 | Zr |
Ba | N/A | -2.75 | -0.04 | ... | -2.80 | -0.04 | -0.62 | Ba |
La | N/A | -2.75 | -0.04 | ... | -2.68 | -0.04 | -1.58 | La |
Eu | N/A | -2.41 | 0.30 | ... | -2.42 | 0.30 | -1.90 | Eu |
Pb | N/A | <-1.43 | <1.28 | ... | <-1.41 | <1.28 | <0.63 | Pb |
Position
Right Ascension : 01 14 06.48 | Declination : -11 02 35.4 | 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 | WHTUES | 52000 | 41 | N/A | N/A |