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A Deep View into the Nucleus of the Sagittarius Dwarf Spheroidal Galaxy with MUSE. I. Data and Stellar Population Characterization

Alfaro-Cuello, M, Kacharov, N, Neumayer, N, Luetzgendorf, N, Seth, AC, Boeker, T, Kamann, S, Leaman, R, van de Ven, G, Bianchini, P, Watkins, LL and Lyubenova, M (2019) A Deep View into the Nucleus of the Sagittarius Dwarf Spheroidal Galaxy with MUSE. I. Data and Stellar Population Characterization. Astrophysical Journal, 886 (1). ISSN 0004-637X

1909.10529v1.pdf - Accepted Version

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The center of the Sagittarius dwarf spheroidal galaxy (Sgr dSph) hosts a nuclear star cluster (NSC), M54, which is the only galaxy nucleus that can be resolved into individual stars at optical wavelengths. It is thus a key target for understanding the formation of NSCs and their relation to globular clusters (GCs). We present a large Multi-Unit Spectroscopic Explorer data set that covers M54 out to ~2.5 half-light radius, from which we extracted the spectra of ~6600 cluster member stars. We use these data in combination with Hubble Space Telescope photometry to derive age and metallicity for each star. The stellar populations show a well-defined age–metallicity relation, implying an extended formation history for the central region of Sgr dSph. We classify these populations into three groups, all with the same systemic velocity: young metal-rich (YMR; 2.2 Gyr, [Fe/H] = −0.04); intermediate-age metal-rich (IMR; 4.3 Gyr, [Fe/H] = −0.29); and old metal-poor (OMP; 12.2 Gyr, [Fe/H] = −1.41). The YMR and OMP populations are more centrally concentrated than the IMR population, which are likely stars of the Sgr dSph. We suggest that the OMP population is the result of accretion and merging of two or more old and metal-poor GCs dragged to the center by dynamical friction. The YMR is consistent with being formed by in situ star formation in the nucleus. The ages of the YMR population suggest that it may have been triggered into forming when the Sgr dSph began losing its gas during the most recent interaction with the Milky Way, ~3 Gyr ago.

Item Type: Article
Uncontrolled Keywords: 0201 Astronomical and Space Sciences, 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics, 0306 Physical Chemistry (incl. Structural)
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: American Astronomical Society; IOP Publishing
Related URLs:
Date Deposited: 26 Jan 2021 10:24
Last Modified: 04 Sep 2021 06:04
DOI or ID number: 10.3847/1538-4357/ab1b2c
URI: https://researchonline.ljmu.ac.uk/id/eprint/14325
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