BS17587-003
ABUNDANCES OF EXTREMELY METAL-POOR STAR CANDIDATES
Teff : 5869 | log g : 3.64 |
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 | N/A | ... | 0.22 | ... | -0.21 | 0.20 | 7.39 | Mg I |
Ca I | N/A | ... | 0.19 | ... | -0.20 | 0.21 | 6.14 | Ca I |
Ti II | N/A | ... | 0.19 | ... | -0.15 | 0.26 | 4.80 | Ti II |
Cr I | N/A | ... | 0.12 | ... | -0.26 | 0.15 | 5.38 | Cr I |
Fe I | N/A | -0.41 | ... | ... | -0.41 | ... | 7.09 | Fe I |
Ba II | N/A | ... | 0.01 | ... | -0.45 | -0.04 | 1.73 | Ba II |
Vrad | 1 |
Right Ascension : 09 39 42.49 | Declination : -13 12 38.4 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2003-04-23 | N/A | KECKII | 7000 | 150 | 600 | N/A |