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Date and Time of the Query: 2019-03-26 T08:09:11 PDT
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For refcode 2009MNRAS.392..879G:
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Copyright by Royal Astronomical Society. 2009MNRAS.392..879G Globular cluster systems in nearby dwarf galaxies - I. HST/ACS observations and dynamical properties of globular clusters at low environmental density Georgiev, Iskren Y.; Puzia, Thomas H.; Hilker, Michael; Goudfrooij, Paul Abstract. We investigate the old globular cluster (GC) population of 68 faint (M_V_ > -16mag) dwarf galaxies located in the halo regions of nearby (<~12Mpc) loose galaxy groups and in the field environment based on archival Hubble Space Telescope (HST)/Advanced Camera for Surveys (ACS) images in F606W and F814W filters. The combined colour distribution of 175 GC candidates peaks at (V - I) = 0.96 +/- 0.07mag and the GC luminosity function turnover for the entire sample is found at M_V,TO_ = -7.6 +/- 0.11mag, similar to the old metal-poor Large Magellanic Cloud (LMC) GC population. Our data reveal a tentative trend of M_V,TO_ becoming fainter from late- to early-type galaxies. The luminosity and colour distributions of GCs in dIrrs show a lack of faint blue GCs (bGCs). Our analysis reveals that this might reflect a relatively younger GC system than typically found in luminous early-type galaxies. If verified by spectroscopy, this would suggest a later formation epoch of the first metal-poor star clusters in dwarf galaxies. We find several bright (massive) GCs which reside in the nuclear regions of their host galaxies. These nuclear clusters have similar luminosities and structural parameters as the peculiar Galactic clusters suspected of being the remnant nuclei of accreted dwarf galaxies, such as M54 and omegaCen. Except for these nuclear clusters, the distribution of GCs in dIrrs in the half-light radius versus cluster mass plane is very similar to that of Galactic young halo clusters, which suggests comparable formation and dynamical evolution histories. A comparison with theoretical models of cluster disruption indicates that GCs in low-mass galaxies evolve dynamically as self-gravitating systems in a benign tidal environment. Key words: galaxies: dwarf, galaxies: irregular, galaxies: star clusters =========================================================================== 2010MNRAS.409..447G Erratum: Globular cluster systems in nearby dwarf galaxies - I. HST/ACS observations and dynamical properties of globular clusters at low environmental density Georgiev, Iskren Y.; Puzia, Thomas H.; Hilker, Michael; Goudfrooij, Paul Abstract. The paper 'Globular cluster systems in nearby dwarf galaxies - I. HST/ACS observations and dynamical properties of globular clusters at low environmental density' was published in Mon. Not. R. Astron. Soc. 392, 879-893 (2009). Owing to confusion with reading tables from literature sources, we erroneously plotted in Fig. 5 the reddening-uncorrected V-I colour of the old Large Magellanic Cloud (LMC) clusters. The reddening-corrected values are bluer by only about 0.1 mag. The only change to the paper is an updated Fig. 5, {see text}. This has no implications for the main results of the paper, and no changes to the text are necessary as there is no discussion regarding the V-I colour of LMC globular clusters (GCs). Key words: errata, addenda, galaxies:dwarf, galaxies:irregular, galaxies:star clusters:general ===========================================================================
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