The Chemical Composition of Giants in the Globular Cluster ω Cen

Verne V. Smith
1988 Symposium - International astronomical union  
High-resolution, high S/N spectra have been obtained for 22 giant stars in the globular cluster ω Cen. These stars span a wide range of temperature and position on the giant branch and include some of the S-type and Barium star members. Spectra were obtained on the CTIO 4m telescope with the echelle spectrograph and CCD detector. Initial abundance results for Iron, Calcium, and Oxygen are presented for three stars: one of the most luminous cluster red-giants, a giant on the blue edge of the ω Cen giant branch, and an extreme Barium star member.
doi:10.1017/s0074180900035646 fatcat:li2oxji6nrfzbnbsx5nod4thia