The age-metallicity degeneracy in the dwarf spheroidal Carina as seen by FLAMES

Koch, Andreas and Grebel, E. K. and Wyse, Rosemary F. G. and Kleyna, Jan and Wilkinson, M. I. and Harbeck, Daniel and Gilmore, G. and Evans, N. W. (2006) The age-metallicity degeneracy in the dwarf spheroidal Carina as seen by FLAMES. The Messenger (123). pp. 38-40. ISSN 0722-6691

Full text not available from this repository.

Abstract

The Carina dwarf spheroidal galaxy is the only one of this type to show clearly episodic star formation separated by long pauses. Still its Red Giant Branch is remarkably narrow. Our medium-resolution spectroscopy of 437 Red Giants in this galactic satellite with FLAMES reveals a full range of metallicities from ~ –3.0 up to ~ 0.0 dex. There also appears to be a mild radial gradient in that more metal-rich populations are more centrally concentrated, matching a similar trend in ages with an increasing fraction of intermediate-age stars in the centre (Harbeck et al. 2001). Complemented by the colours of the more metal-rich stars, this suggests that Carina exhibits an age-metallicity relation. We address the star formation in this intriguing galaxy by also pursuing its agemetallicity degeneracy, resulting in a narrow Red Giant Branch despite the considerable spread in metallicity and wide range of ages, and applying basic models of chemical evolution.

Item Type: Journal Article
Journal or Publication Title: The Messenger
Departments: Faculty of Science and Technology > Physics
ID Code: 83643
Deposited By: ep_importer_pure
Deposited On: 14 Dec 2016 16:36
Refereed?: No
Published?: Published
Last Modified: 12 Dec 2019 04:10
URI: https://eprints.lancs.ac.uk/id/eprint/83643

Actions (login required)

View Item View Item