The globular cluster system of NGC 1316. II - The extraordinary object SH2
Abstract
SH2 has been described as an isolated HII-region, located about 6.5 arcmin south of the nucleus of NGC 1316 (Fornax A), a merger remnant in the the outskirts of the Fornax cluster of galaxies. We give a first, preliminary description of the stellar content and environment of this remarkable object. We used photometric data in the Washington system and HST photometry from the Hubble Legacy Archive for a morphological description and preliminary aperture photometry. Low-resolution spectroscopy provides radial velocities of the brightest star cluster in SH2 and a nearby intermediate-age cluster. SH2 is not a normal HII-region, ionized by very young stars. It contains a multitude of star clusters with ages of approximately 0.1 Gyr. A ring-like morphology is striking. SH2 seems to be connected to an intermediate-age massive globular cluster with a similar radial velocity, which itself is the main object of a group of fainter clusters. Metallicity estimates from emission lines remain ambiguous. The present data do not yet allow firm conclusions about the nature or origin of SH2. It might be a dwarf galaxy that has experienced a burst of extremely clustered star formation. We may witness how globular clusters are donated to a parent galaxy.
Keywords
Cite
@article{arxiv.1203.2463,
title = {The globular cluster system of NGC 1316. II - The extraordinary object SH2},
author = {T. Richtler and B. Kumar and L. P. Bassino and B. Dirsch and A. J. Romanowsky},
journal= {arXiv preprint arXiv:1203.2463},
year = {2015}
}
Comments
5 pages, to appear in A&A, format slightly different from the printed version