BD+20_2030: found in 2 paper(s).
Labels:
/E.Arnone et al.(2005)/
/A.Hosford et al.(2009)/
Find this object in SIMBAD

A0075
| Title | Mg abundances in metal-poor halo stars as a tracer of early Galactic mixing |
| ADS | E.Arnone et al.,AAP, 430, 507, 2005 |
| Authors | E. Arnone, S. G. Ryan, D. Argast, J. E. Norris, T. C. Beers |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | ANGLO | 40000 | >100 | N/A | N/A |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 6200 |
| log g | 3.9+-0.2 |
| vturb | 1.6+-0.2 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| Mg I | ... | -2.39+-0.06 | 0.29+-0.06 | 5.19+-0.06 |
| Ca I | ... | -2.23+-0.04 | 0.45+-0.04 | 4.13+-0.04 |
| Ti I | ... | -2.16 | 0.52 | 2.86 |
| Cr I | ... | -2.62+-0.04 | 0.06+-0.04 | 3.05+-0.04 |
| Fe I | ... | -2.68+-0.01 | ... | 4.82+-0.01 |
| Fe II | ... | -2.68 | ... | 4.82 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0169
| Title | Lithium abundances of halo dwarfs based on excitation temperature. I. Local thermodynamic equilibrium |
| ADS | A.Hosford et al.,AAP, 493, 601, 2009 |
| Authors | A. Hosford, S. G. Ryan, A. E. GarciaPerez, J. E. Norris, K. A. Olive |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | N/A | ANGLO | 43000 | 95 | N/A | N/A |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | 195124 |
| Right Ascension | 081313 |
Photometric data
Atmospheric data
| Teff | 6208+-104 |
| log g | 4.46+-0.14 |
| vturb | 1.00 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| Li I | ... | 0.95+-0.068 | 3.58+-0.068 | 2.11+-0.068 |
| Fe | ... | -2.63 | ... | 4.87 |
| Fe I | ... | -2.62 | ... | 4.88 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)