Differential chemical abundance analysis of a 47 Tucanæ asymptotic giant branch star with respect to Arcturus
This study resolves a discrepancy in the abundance of Zr in the 47 Tucanæ asymptotic giant branch (AGB) star Lee 2525. This star was observed using the echelle spectrograph on the 2.3-m telescope at Siding Spring Observatory. The analysis was undertaken
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Worley_Differential_chemical_2009.pdf||734.96 kB||Adobe PDF||Request a copy|
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