BD+20_2030
/E.Arnone et al.(2005)/ /A.Hosford et al.(2009)/ /J.A.Rich and A. M. Boesgaard(2009)/ /A.M.Boesgaard et al.(2011)/
Mg abundances in metal-poor halo stars as a tracer of early Galactic mixing
Teff : 6200 | log g : 3.9+-0.2 | vturb : 1.6+-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 |
Mg I | 3 | -2.39+-0.06 | 0.29+-0.06 | ... | -2.41+-0.06 | 0.27+-0.06 | 5.19+-0.06 | Mg I |
Ca I | 3 | -2.23+-0.04 | ... | ... | -2.21+-0.04 | 0.47+-0.04 | 4.13+-0.04 | Ca I |
Ti I | 1 | -2.16 | ... | ... | -2.09 | 0.59 | 2.86 | Ti I |
Cr I | 2 | -2.62+-0.04 | ... | ... | -2.59+-0.04 | 0.09+-0.04 | 3.05+-0.04 | Cr I |
Fe I | 16 | -2.68+-0.01 | ... | ... | -2.68+-0.01 | ... | 4.82+-0.01 | Fe I |
Fe II | 1 | -2.68 | ... | ... | -2.68 | ... | 4.82 | Fe II |
Right Ascension : 08 16 07.35 | Declination : +19 41 51.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
N/A | ANGLO | 40000 | >100 | N/A | N/A |
Lithium abundances of halo dwarfs based on excitation temperature. I. Local thermodynamic equilibrium
Teff : 6208+-104 | log g : 4.46+-0.14 | vturb : 1.00 |
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 | ... | ... | 2.11+-0.068 | -1.15+-0.068 | 1.48+-0.068 | 2.11+-0.068 | Li I |
Fe | N/A | -2.63 | ... | ... | -2.63 | ... | 4.87 | Fe |
Fe I | 98 | -2.62 | ... | ... | -2.62 | ... | 4.88 | Fe I |
Right Ascension : 08 16 07.35 | Declination : +19 41 51.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
N/A | N/A | ANGLO | 43000 | 95 | N/A | N/A |
BERYLLIUM, OXYGEN, AND IRON ABUNDANCES IN EXTREMELY METAL-DEFICIENT STARS
Teff : 5978 | log g : 3.61 |
Original Data | Converted Data Asplund et al. (2009) | |||||||
---|---|---|---|---|---|---|---|---|
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Be II | N/A | ... | ... | -1.23+-0.12 | -2.61+-0.12 | 0.16+-0.12 | -1.23+-0.12 | Be II |
OH | N/A | -2.06+-0.14 | ... | ... | -1.88+-0.14 | 0.89+-0.14 | 6.81+-0.14 | OH |
Fe | N/A | -2.77+-0.1 | ... | ... | -2.77+-0.1 | ... | 4.73+-0.1 | Fe |
Right Ascension : 08 16 07.35 | Declination : +19 41 51.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2006-01-02 | N/A | KECKHIRES | 48000 | 122 | 3600 | N/A |
Beryllium and Alpha-element Abundances in a Large Sample of Metal-poor Stars
Teff : 5978+-100 | log g : 3.61+-0.2 | vturb : 1.5+-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 |
Be | N/A | ... | +0.12+-0.15 | -1.23+-0.12 | -2.61+-0.12 | 0.16+-0.15 | -1.23+-0.12 | Be |
O | N/A | -2.06+-0.22 | +0.71+-0.24 | ... | -2.12+-0.22 | 0.65+-0.24 | 6.57+-0.22 | O |
Mg | N/A | -2.29+-0.07 | ... | ... | -2.31+-0.07 | 0.46+-0.07 | 5.29+-0.07 | Mg |
Ti | N/A | -2.24+-0.09 | ... | ... | -2.17+-0.09 | 0.60+-0.09 | 2.78+-0.09 | Ti |
Fe | N/A | -2.77+-0.09 | ... | ... | -2.77+-0.09 | ... | 4.73+-0.09 | Fe |
Right Ascension : | Declination : | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
N/A | KECKHIRES | 42000 | N/A | N/A | N/A |