HE0212-0557
/J.G.Cohen et al.(2006)/ /J.G.Cohen et al.(2013)/
Carbon Stars in the Hamburg/ESO Survey: Abundances
Teff : 5075 | log g : 2.15 | vturb : 1.8 |
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 | ... | 1.74 | 8.06 | -0.37 | 1.95 | 8.06 | CH |
CN | 1 | ... | 1.09 | 6.75 | -1.08 | 1.24 | 6.75 | CN |
Mg I | 1 | ... | 0.04 | 5.32 | -2.28 | 0.04 | 5.32 | Mg I |
Al I | 1 | ... | 0.01 | 4.21 | -2.24 | 0.08 | 4.21 | Al I |
Ca I | 1 | ... | 0.14 | 4.23 | -2.11 | 0.21 | 4.23 | Ca I |
Ti I | 5 | ... | 0.14+-0.32 | 2.87+-0.32 | -2.08+-0.32 | 0.24+-0.32 | 2.87+-0.32 | Ti I |
Ti II | 8 | ... | 0.32+-0.32 | 3.04+-0.32 | -1.91+-0.32 | 0.41+-0.32 | 3.04+-0.32 | Ti II |
Cr I | 2 | ... | -0.09+-0.03 | 3.31+-0.03 | -2.33+-0.03 | -0.01+-0.03 | 3.31+-0.03 | Cr I |
Mn I | 4 | ... | -0.55+-0.46 | 2.57+-0.46 | -2.86+-0.46 | -0.54+-0.46 | 2.57+-0.46 | Mn I |
Fe I | 17 | -2.27+-0.26 | ... | 5.18+-0.26 | -2.32+-0.26 | ... | 5.18+-0.26 | Fe I |
Fe II | 7 | ... | 0.04+-0.28 | 5.23+-0.28 | -2.27+-0.28 | 0.04+-0.28 | 5.23+-0.28 | Fe II |
Sr II | 1 | ... | -0.05 | 0.59 | -2.28 | 0.04 | 0.59 | Sr II |
Y II | 3 | ... | 0.55+-0.16 | 0.53+-0.16 | -1.68+-0.16 | 0.64+-0.16 | 0.53+-0.16 | Y II |
Ba II | 2 | ... | 2.18+-0.06 | 2.04+-0.06 | -0.14+-0.06 | 2.18+-0.06 | 2.04+-0.06 | Ba II |
La II | 3 | ... | 2.28+-0.22 | 1.15+-0.22 | 0.05+-0.22 | 2.37+-0.22 | 1.15+-0.22 | La II |
Ce II | 1 | ... | 2.14 | 1.42 | -0.16 | 2.16 | 1.42 | Ce II |
Pr II | 1 | ... | 2.37 | 0.81 | 0.09 | 2.41 | 0.81 | Pr II |
Nd II | 1 | ... | 1.90 | 1.13 | -0.29 | 2.03 | 1.13 | Nd II |
Vrad | -230.6 |
Right Ascension : 02 15 02.50 | Declination : -05 43 23.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
N/A | KECKHIRES | 45000 | 100 | 6000 | N/A |
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
Teff : 5075+-100 | log g : 2.2+-0.25 | vturb : 1.8+-0.2 |
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 | ... | 1.74 | ... | -0.37 | 1.95 | 8.06 | CH |
NH | 1 | ... | 1.09 | ... | -1.08 | 1.24 | 6.75 | NH |
Mg I | 1 | ... | 0.04 | ... | -2.29 | 0.03 | 5.31 | Mg I |
Al I | 1 | ... | 0.01 | ... | -2.24 | 0.08 | 4.21 | Al I |
Ca I | 1 | ... | 0.14 | ... | -2.11 | 0.21 | 4.23 | Ca I |
Ti I | 5 | ... | 0.14+-0.32 | ... | -2.09+-0.32 | 0.23+-0.32 | 2.86+-0.32 | Ti I |
Ti II | 8 | ... | 0.32+-0.32 | ... | -1.91+-0.32 | 0.41+-0.32 | 3.04+-0.32 | Ti II |
Cr I | 2 | ... | -0.09+-0.03 | ... | -2.33+-0.03 | -0.01+-0.03 | 3.31+-0.03 | Cr I |
Mn I | 4 | ... | -0.55+-0.46 | ... | -2.86+-0.46 | -0.54+-0.46 | 2.57+-0.46 | Mn I |
Fe I | N/A | -2.27+-0.26 | ... | ... | -2.32+-0.26 | ... | 5.18+-0.26 | Fe I |
Fe II | 7 | -2.23+-0.28 | 0.04+-0.28 | ... | -2.28+-0.28 | 0.04+-0.28 | 5.22+-0.28 | Fe II |
Sr II | 1 | ... | -0.05 | ... | -2.29 | 0.03 | 0.58 | Sr II |
Y II | 3 | ... | 0.55+-0.16 | ... | -1.69+-0.16 | 0.63+-0.16 | 0.52+-0.16 | Y II |
Ba II | 2 | ... | 2.18+-0.06 | ... | -0.14+-0.06 | 2.18+-0.06 | 2.04+-0.06 | Ba II |
La II | 3 | ... | 2.28+-0.22 | ... | 0.05+-0.22 | 2.37+-0.22 | 1.15+-0.22 | La II |
Ce II | 1 | ... | 2.14 | ... | -0.16 | 2.16 | 1.42 | Ce II |
Pr II | 1 | ... | 2.37 | ... | 0.09 | 2.41 | 0.81 | Pr II |
Nd II | 1 | ... | 1.64 | ... | -0.55 | 1.77 | 0.87 | Nd II |
Vrad | -230.6 |
Right Ascension : 02 15 02.50 | Declination : -05 43 23.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2002-09 | N/A | KECKHIRES | 36000 | 105 | 6000 | -230.6 |