BS17587-016
ABUNDANCES OF EXTREMELY METAL-POOR STAR CANDIDATES
Teff : 6014 | log g : 3.71 |
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 | ... | 0.28 | ... | -0.01 | 0.26 | 7.59 | Mg I |
Ca I | N/A | ... | 0.19 | ... | -0.06 | 0.21 | 6.28 | Ca I |
Ti II | N/A | ... | 0.10 | ... | -0.10 | 0.17 | 4.85 | Ti II |
Cr I | N/A | ... | -0.17 | ... | -0.41 | -0.14 | 5.23 | Cr I |
Fe I | N/A | -0.27 | ... | ... | -0.27 | ... | 7.23 | Fe I |
Ba II | N/A | ... | -0.10 | ... | -0.42 | -0.15 | 1.76 | Ba II |
Vrad | -18 |
Right Ascension : 09 40 33.27 | Declination : -13 23 29.5 | 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 |