The Chemical Composition of Giants in the Globular Cluster ω Cen release_li2oxji6nrfzbnbsx5nod4thia

by Verne V. Smith

Published in Symposium - International astronomical union by Cambridge University Press (CUP).

1988   Volume 132, p541-544

Abstract

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.
In application/xml+jats format

Archived Files and Locations

application/pdf   478.5 kB
file_crujbl6tjfayllu7k2hduumy5y
application/pdf   478.5 kB
file_kzrclb2debahzaf3mcsirssc5y
www.cambridge.org (web)
web.archive.org (webarchive)
Read Archived PDF
Preserved and Accessible
Type  article-journal
Stage   published
Year   1988
Language   en ?
Container Metadata
Not in DOAJ
In Keepers Registry
ISSN-L:  0074-1809
Work Entity
access all versions, variants, and formats of this works (eg, pre-prints)
Catalog Record
Revision: e0682af2-c4d9-4e51-aed4-a61e0b37edf6
API URL: JSON