A blue tilt in the globular cluster system of the Milky Way-like galaxy NGC 5170

D.A. Forbes, L. R. Spitler, W.E. Harris, J. Bailin, J. Strader, J.P. Brodie, S.S. Larsen

    Research output: Contribution to journalArticleAcademicpeer-review

    Abstract

    Here, we present Hubble Space Telescope/Advanced Camera for Surveys (ACS) imaging, in the B and I bands, of the edge-on Sb/Sc galaxy NGC 5170. Excluding the central disc region, we detect 142 objects with colours and sizes typical of globular clusters (GCs). Our main result is the discovery of a ‘blue tilt’ (a mass–metallicity relation), at the 3σ level, in the metal-poor GC subpopulation of this Milky Way like galaxy. The tilt is consistent with that seen in massive elliptical galaxies and with the self-enrichment model of Bailin & Harris. For a linear mass–metallicity relation, the tilt has the form Z ∼ L0.42±0.13. We derive a total GC system population of 600 ± 100, making it much richer than the Milky Way. However, when this number is normalized by the host galaxy luminosity or stellar mass it is similar to that of M31. Finally, we report the presence of a potential Ultra Compact Dwarf of size ∼6 pc and luminosity MI ∼−12.5, assuming it is physically associated with NGC 5170.
    Original languageEnglish
    Pages (from-to)429-438
    Number of pages10
    JournalMonthly Notices of the Royal Astronomical Society
    Volume403
    Issue number1
    DOIs
    Publication statusPublished - 2010

    Keywords

    • globular clusters: general
    • galaxies: individual: NGC 5170
    • galaxies: star clusters

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