A close look at the Centaurus A group of galaxies:I. Metallicity distribution functions and population gradients in early-type dwarfs

Crnojevic, D. and Grebel, E.K. and Koch, Andreas (2010) A close look at the Centaurus A group of galaxies:I. Metallicity distribution functions and population gradients in early-type dwarfs. Astronomy and Astrophysics, 516. ISSN 1432-0746

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Abstract

Aims. We study dwarf galaxies in the Centaurus A group to investigate their metallicity and possible environmental effects. The Centaurus A group (at ~4 Mpc from the Milky Way) contains about 50 known dwarf companions of different morphologies and stellar contents, thus making it a very interesting target to study how these galaxies evolve. Methods. Here we present results for the early-type dwarf galaxy population in this group. We used archival HST/ACS data to study the resolved stellar content of 6 galaxies, together with isochrones from the Dartmouth stellar evolutionary models. Results. We derive photometric metallicity distribution functions of stars on the upper red giant branch via isochrone interpolation. The 6 galaxies are moderately metal-poor ([Fe/H] = -1.56 to -1.08), and metallicity spreads are observed (internal dispersions of σ[Fe/H] = 0.10–0.41 dex). We also investigate whether intermediate-age stars are present, and discuss how these affect our results. The dwarfs exhibit flat to weak radial metallicity gradients. For the two most luminous, most metal-rich galaxies, we find statistically significant evidence of at least two stellar subpopulations: the more metal-rich stars are found in the center of the galaxies, while the metal-poor ones are more broadly distributed within the galaxies. Conclusions. We find no clear trend in the derived physical properties as a function of (present-day) galaxy position in the group, which may come from the small sample we investigate. We compare our results to the early-type dwarf population of the Local Group, and find no outstanding differences, even though the Centaurus A group is a denser environment that is possibly in a more advanced dynamical stage.

Item Type: Journal Article
Journal or Publication Title: Astronomy and Astrophysics
Uncontrolled Keywords: /dk/atira/pure/subjectarea/asjc/1900/1912
Subjects:
Departments: Faculty of Science and Technology > Physics
ID Code: 83397
Deposited By: ep_importer_pure
Deposited On: 02 Dec 2016 15:12
Refereed?: Yes
Published?: Published
Last Modified: 01 Jan 2020 10:06
URI: https://eprints.lancs.ac.uk/id/eprint/83397

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