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s- and r-Process Element Abundances in the CMD of 47 Tucanæ Using the Robert Stobie Spectrograph on SALT*

C. C. Worley A C , P. L. Cottrell A and E. C. Wylie de Boer B
+ Author Affiliations
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A Department of Physics & Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand

B Research School of Astronomy & Astrophysics, Mount Stromlo Observatory, Cotter Rd, Weston, ACT 2611, Australia

C Corresponding author. Email: clare.worley@pg.canterbury.ac.nz

Publications of the Astronomical Society of Australia 25(2) 53-62 https://doi.org/10.1071/AS07031
Submitted: 27 August 2007  Accepted: 21 December 2007   Published: 26 June 2008



2 articles found in Crossref database.

Differential chemical abundance analysis of a 47 Tucan�� asymptotic giant branch star with respect to Arcturus
Worley C. C., Cottrell P. L., Freeman K. C., Wylie-de Boer E. C.
Monthly Notices of the Royal Astronomical Society. 2009 400(2). p.1039
Medium-Resolution s-process Element Survey of 47 Tuc Giant Stars
Worley C. C., Cottrell P. L.
Publications of the Astronomical Society of Australia. 2012 29(1). p.29
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