BPS CS22941-012: found in 2 paper(s).
Labels:
/C.Sneden et al.(2003)/
/G.W.Preston et al.(2000)/
Find this object in SIMBAD

A0020
| Title | Binary Blue Metal-poor Stars: Evidence for Asymptotic Giant Branch Mass Transfer |
| ADS | C.Sneden et al.,ApJ, 592, 504, 2003 |
| Authors | C. Sneden, G. W. Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101, . Preston, J. J. Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, . Cowan |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | 2452122.87 | FRUTTI | 30000 | N/A | N/A | -121.6 |
| N/A | 2452123.8 | FRUTTI | 30000 | N/A | N/A | -122.4 |
| N/A | 2452124.81 | FRUTTI | 30000 | N/A | N/A | -122.5 |
| N/A | 2452474.83 | FRUTTI | 30000 | N/A | N/A | -122.5 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
| V | 12.5 |
| B-V | 0.28 |
| U-B | -0.17 |
Atmospheric data
| Teff | 7200 |
| log g | 4.2 |
| vturb | 2.50 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| CH | ... | -1.03+-0.3 | +1.0+-0.3 | 7.52+-0.3 |
| O I | ... | -1.63+-0.28 | +0.40+-0.28 | 7.24+-0.28 |
| Fe | ... | -2.03 | ... | 5.47 |
| Sr II | ... | -2.10+-0.10 | -0.07+-0.10 | 0.87+-0.10 |
| Ba II | ... | -1.87 | +0.16 | 0.26 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0045
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | 2448812.771 | FRUTTI | 30000 | 10 | N/A | -123.1 |
| N/A | 2448824.755 | FRUTTI | 30000 | 10 | N/A | -122.5 |
| N/A | 2449194.745 | FRUTTI | 30000 | 10 | N/A | -122.2 |
| N/A | 2449573.751 | FRUTTI | 30000 | 10 | N/A | -122.7 |
| N/A | 2449577.684 | FRUTTI | 30000 | 10 | N/A | -121.8 |
| N/A | 2449578.739 | FRUTTI | 30000 | 10 | N/A | -121.5 |
| N/A | 2449581.741 | FRUTTI | 30000 | 10 | N/A | -122.1 |
| N/A | 2449582.79 | FRUTTI | 30000 | 10 | N/A | -123.5 |
| N/A | 2449583.819 | FRUTTI | 30000 | 10 | N/A | -122.5 |
| N/A | 2449584.669 | FRUTTI | 30000 | 10 | N/A | -122.7 |
| N/A | 2449588.711 | FRUTTI | 30000 | 10 | N/A | -121.6 |
| N/A | 2449590.691 | FRUTTI | 30000 | 10 | N/A | -123.4 |
| N/A | 2449936.716 | FRUTTI | 30000 | 10 | N/A | -122.9 |
| N/A | 2449938.819 | FRUTTI | 30000 | 10 | N/A | -121.9 |
| N/A | 2450290.668 | FRUTTI | 30000 | 10 | N/A | -122.3 |
| N/A | 2450296.681 | FRUTTI | 30000 | 10 | N/A | -123.1 |
| N/A | 2450646.708 | FRUTTI | 30000 | 10 | N/A | -122.9 |
| N/A | 2450703.708 | FRUTTI | 30000 | 10 | N/A | -123.7 |
| N/A | 2450704.666 | FRUTTI | 30000 | 10 | N/A | -122.3 |
| N/A | 2450705.627 | FRUTTI | 30000 | 10 | N/A | -122.1 |
| N/A | 2450706.777 | FRUTTI | 30000 | 10 | N/A | -122.2 |
| N/A | 2450707.744 | FRUTTI | 30000 | 10 | N/A | -121.5 |
| N/A | 2450997.807 | FRUTTI | 30000 | 10 | N/A | -122.4 |
| N/A | 2450998.723 | FRUTTI | 30000 | 10 | N/A | -123.8 |
| N/A | 2451001.827 | FRUTTI | 30000 | 10 | N/A | -121.3 |
| N/A | 2451002.73 | FRUTTI | 30000 | 10 | N/A | -121.7 |
| N/A | 2451032.657 | FRUTTI | 30000 | 10 | N/A | -122.2 |
| N/A | 2451358.893 | FRUTTI | 30000 | 10 | N/A | -122.3 |
| N/A | 2451360.791 | FRUTTI | 30000 | 10 | N/A | -122.0 |
| N/A | 2451384.741 | FRUTTI | 30000 | 10 | N/A | -122.0 |
| N/A | 2451386.727 | FRUTTI | 30000 | 10 | N/A | -121.8 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
| V | 12.5 |
| B-V | 0.28 |
| U-B | -0.17 |
Atmospheric data
| Teff | 7200 |
| log g | 4.20 |
| vturb | 2.50 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| Mg I | ... | -1.72 | 0.31 | 5.86 |
| Ca I | ... | -1.58 | 0.45 | 4.78 |
| Sc II | ... | -1.68 | 0.35 | 1.49 |
| Ti II | ... | -1.48 | 0.55 | 3.54 |
| Cr I | ... | -2.10 | -0.07 | 3.57 |
| Mn I | ... | -2.24 | -0.21 | 3.15 |
| Fe | ... | -2.03 | ... | 5.47 |
| Sr II | ... | -2.07 | -0.04 | 0.90 |
| Ba II | ... | -1.90 | 0.13 | 0.23 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)