HE1152-0355
/A.Goswami et al.(2006)/ /A.Susmitha et al.(2021)/
A high-resolution spectral analysis of three carbon-enhanced metal-poor stars
Teff : 4000 | log g : 1.0 | vturb : 2.0 |
Original Data | Converted Data Asplund et al. (2009) | |||||||
---|---|---|---|---|---|---|---|---|
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
C I | N/A | -0.69 | 0.58 | 7.7 | -0.73 | 0.59 | 7.7 | C I |
Mg I | N/A | -1.28 | -0.01 | 6.25 | -1.35 | -0.03 | 6.25 | Mg I |
Ti II | N/A | -0.75 | 0.52 | 4.15 | -0.80 | 0.52 | 4.15 | Ti II |
Fe I | N/A | -1.27 | ... | 6.18+-0.27 | -1.32 | ... | 6.18+-0.27 | Fe I |
Fe II | N/A | -1.3 | ... | 6.15+-0.24 | -1.35 | ... | 6.15+-0.24 | Fe II |
Y II | N/A | -1.16 | 0.14 | 1.05 | -1.16 | 0.16 | 1.05 | Y II |
Zr I | N/A | -1.27 | 0.0 | 1.32 | -1.26 | 0.06 | 1.32 | Zr I |
Ba II | N/A | 0.28 | 1.58 | 2.45 | 0.27 | 1.59 | 2.45 | Ba II |
La II | N/A | 0.27 | 1.57 | 1.4 | 0.30 | 1.62 | 1.4 | La II |
Nd II | N/A | -0.87 | 0.43 | 0.58 | -0.84 | 0.48 | 0.58 | Nd II |
Sm II | N/A | -0.43 | 0.87 | 0.58 | -0.38 | 0.94 | 0.58 | Sm II |
Vrad | +431.3+-1.5 |
Right Ascension : 11 55 06.06 | Declination : -04 12 24.7 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2003-3-25 | 2452784.83629 | SUBARUHDS | 50000 | N/A | 600 | N/A |
Optical and NIR spectroscopy of cool CEMP stars to probe the nucleosynthesis in low-mass AGB binary system
Teff : 4200+-150 | log g : 0.25+-0.25 | vturb : 2.2+-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 |
Li I | N/A | ... | <0.00+-0.30 | ... | <0.00+-0.30 | <0.00+-0.30 | <3.26+-0.30 | Li I |
C2 | N/A | ... | 1.35+-0.20 | ... | 1.35+-0.20 | 1.35+-0.20 | 9.78+-0.20 | C2 |
CN | N/A | ... | 0.95+-0.20 | ... | 0.95+-0.20 | 0.95+-0.20 | 8.78+-0.20 | CN |
[O I] | N/A | ... | 0.50+-0.30 | ... | 0.50+-0.30 | 0.50+-0.30 | 9.19+-0.30 | [O I] |
Na I | N/A | ... | -0.10+-0.20 | ... | -0.10+-0.20 | -0.10+-0.20 | 6.14+-0.20 | Na I |
Mg I | N/A | ... | 0.40+-0.20 | ... | 0.40+-0.20 | 0.40+-0.20 | 8.00+-0.20 | Mg I |
Al I | N/A | ... | <-0.20+-0.30 | ... | <-0.20+-0.30 | <-0.20+-0.30 | <6.25+-0.30 | Al I |
K I | N/A | ... | 0.70+-0.20 | ... | 0.70+-0.20 | 0.70+-0.20 | 5.73+-0.20 | K I |
Ca I | N/A | ... | 0.30+-0.30 | ... | 0.30+-0.30 | 0.30+-0.30 | 6.64+-0.30 | Ca I |
Sc II | N/A | ... | 0.00+-0.20 | ... | 0.00+-0.20 | 0.00+-0.20 | 3.15+-0.20 | Sc II |
Rb I | N/A | ... | <-0.30+-0.20 | ... | <-0.30+-0.20 | <-0.30+-0.20 | <2.06+-0.20 | Rb I |
Y II | N/A | ... | 0.40+-0.20 | ... | 0.40+-0.20 | 0.40+-0.20 | 2.61+-0.20 | Y II |
Zr II | N/A | ... | 0.40+-0.20 | ... | 0.40+-0.20 | 0.40+-0.20 | 2.98+-0.20 | Zr II |
Ba II | N/A | ... | 1.30+-0.20 | ... | 1.30+-0.20 | 1.30+-0.20 | 3.48+-0.20 | Ba II |
La II | N/A | ... | 1.40+-0.20 | ... | 1.40+-0.20 | 1.40+-0.20 | 2.50+-0.20 | La II |
Ce II | N/A | ... | 1.20+-0.20 | ... | 1.20+-0.20 | 1.20+-0.20 | 2.78+-0.20 | Ce II |
Pr II | N/A | ... | 1.18+-0.20 | ... | 1.18+-0.20 | 1.18+-0.20 | 1.90+-0.20 | Pr II |
Nd II | N/A | ... | 1.20+-0.20 | ... | 1.20+-0.20 | 1.20+-0.20 | 2.62+-0.20 | Nd II |
Sm II | N/A | ... | 0.90+-0.20 | ... | 0.90+-0.20 | 0.90+-0.20 | 1.86+-0.20 | Sm II |
Eu II | N/A | ... | <0.36+-0.20 | ... | <0.36+-0.20 | <0.36+-0.20 | <0.88+-0.20 | Eu II |
12C/13C | 9+-6 |
Vrad | 428.6 |
Right Ascension : 11 55 06.06 | Declination : -04 12 24.71 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2457802.31004023 | HCTHESP | 30000 | 26.7 | 2700 | 428.6 |