The complex star cluster system of NGC 1316 (Fornax A)

This paper presents Gemini-gri high-quality photometry for cluster candidates in the field of NGC 1316 (Fornax A) as part of a study that also includes GMOS spectroscopy. A preliminary discussion of the photometric data indicates the presence of four stellar cluster populations with distinctive feat...

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Bibliographic Details
Authors: Sesto, Leandro Alberto, Faifer, Favio Raúl, Forte, Juan Carlos
Format: article
Status:Published version
Publication Date:2016
Country:Argentina
Institution:Consejo Nacional de Investigaciones Científicas y Técnicas
Repository:CONICET Digital (CONICET)
Language:English
OAI Identifier:oai:ri.conicet.gov.ar:11336/36097
Online Access:http://hdl.handle.net/11336/36097
Access Level:Open access
Keyword:Galaxies
Elliptical galaxies
Lenticular galaxies
Haloes
Photometry
Star clusters
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
Description
Summary:This paper presents Gemini-gri high-quality photometry for cluster candidates in the field of NGC 1316 (Fornax A) as part of a study that also includes GMOS spectroscopy. A preliminary discussion of the photometric data indicates the presence of four stellar cluster populations with distinctive features in terms of age, chemical abundance and spatial distribution. Two of them seem to be the usually old (metal poor and metal rich) populations typically found in elliptical galaxies. In turn, an intermediate-age (5 Gyr) globular cluster population is the dominant component of the sample (as reported by previous papers). We also find a younger cluster population with a tentative age of ≈ 1 Gyr.