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Stellar populations and star formation histories of the nuclear star clusters in six nearby galaxies
Kacharov, Nikolay; Neumayer, Nadine; Seth, Anil C.; Cappellari, Michele; McDermid, Richard; Walcher, C. Jakob; Böker, Torsten
AA(Max Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany), AB(Max Planck Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany), AC(Department of Physics and Astronomy, University of Utah, 115 South 1400 East, Salt Lake City, Utah 84112, USA), AD(Sub-Department of Astrophysics, Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK 0000-0002-1283-8420), AE(Department of Physics and Astronomy, Macquarie University, Sydney, NSW 2109, Australia; Australian Gemini Office, Australian Astronomical Observatory, PO Box 915, Sydney, NSW 1670, Australia), AF(Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, D-14482, Potsdam, Germany), AG(European Space Agency, c/o STScI, 3700 San Martin Drive, Baltimore, MD 21218, USA)
Monthly Notices of the Royal Astronomical Society, Volume 480, Issue 2, p.1973-1998 (MNRAS Homepage)
Publication Date:
Astronomy Keywords:
techniques: spectroscopic, galaxies: individual: NGC 247, NGC 300, NGC 3621, NGC 5102, NGC 5206, NGC 7793, galaxies: nuclei, galaxies: star formation
Abstract Copyright:
2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Bibliographic Code:


The majority of spiral and elliptical galaxies in the Universe host very dense and compact stellar systems at their centres known as nuclear star clusters (NSC). In this work, we study the stellar populations and star formation histories (SFH) of the NSCs of six nearby galaxies with stellar masses ranging between 2 and 8× 10^9 M_{&sun;} (four late-type spirals and two early-types) with high-resolution spectroscopy. Our observations are taken with the X-shooter spectrograph at the VLT. We make use of an empirical simple stellar population (SSP) model grid to fit composite stellar populations to the data and recover the SFHs of the nuclei. We find that the nuclei of all late-type galaxies experienced a prolonged SFH, while the NSCs of the two early-types are consistent with SSPs. The NSCs in the late-type galaxies sample appear to have formed a significant fraction of their stellar mass already more than 10 Gyr ago, while the NSCs in the two early-type galaxies are surprisingly younger. Stars younger than 100 Myr are present in at least two nuclei: NGC 247 & NGC 7793, with some evidence for young star formation in NGC 300's NSC. The NSCs of the spirals NGC 247 and NGC 300 are consistent with prolonged in situ star formation with a gradual metallicity enrichment from ˜-1.5 dex more than 10 Gyr ago, reaching super-Solar values few hundred Myr ago. NGC 3621 appears to be very metal-rich already in the early Universe and NGC 7793 presents us with a very complex SFH, likely dominated by merging of various massive star clusters coming from different environments.
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