Publication Date
4-1-2022
Document Type
Article
Publication Title
Monthly Notices of the Royal Astronomical Society
Volume
511
Issue
3
DOI
10.1093/mnras/stac258
First Page
3179
Last Page
3197
Abstract
We study the present-day rotational velocity ( V rot ) and velocity dispersion ( ?) profiles of the globular cluster (GC) systems in a sample of 50 lenticular (S0) galaxies from the E-MOSAICS galaxy formation simulations. We find that 82 per cent of the galaxies have GCs that are rotating along the photometric major axis of the galaxy ( aligned ), while the remaining 18 per cent of the galaxies do not ( misaligned ). This is generally consistent with the observations from the SLUGGS surv e y. F or the aligned galaxies, classified as peaked and outwardly decreasing (49 per cent ), flat (24 per cent ), and increasing (27 per cent ) based on the V rot / ?profiles out to large radii, we do not find any clear correlation between these present-day V rot / ?profiles of the GCs and the past merger histories of the S0 galaxies, unlike in previous simulations of galaxy stars. For just over half of the misaligned galaxies, we find that the GC misalignment is the result of a major merger within the last 10 Gyr so that the ex-situ GCs are misaligned by an angle between 0 ?(co-rotation) and 180 ?(counter-rotation), with respect to the in situ GCs, depending on the orbital configuration of the merging galaxies. For the remaining misaligned galaxies, we suggest that the in situ metal-poor GCs, formed at early times, have undergone more frequent kinematic perturbations than the in situ metal-rich GCs. We also find that the GCs accreted early and the in situ GCs are predominantly located within 0.2 virial radii ( R 200 ) from the centre of galaxies in 3D phase-space diagrams.
Funding Number
714907
Funding Sponsor
Horizon 2020 Framework Programme
Keywords
galaxies: elliptical and lenticular, cD, galaxies: formation, galaxies: kinematics and dynamics, galaxies: star clusters: general
Department
Physics and Astronomy
Recommended Citation
Arianna Dolfi, Joel Pfeffer, Duncan A. Forbes, Warrick J. Couch, Kenji Bekki, Jean P. Brodie, Aaron J. Romanowsky, and J. M.Diederik Kruijssen. "The present-day globular cluster kinematics of lenticular galaxies from the E-MOSAICS simulations and their relation to the galaxy assembly histories" Monthly Notices of the Royal Astronomical Society (2022): 3179-3197. https://doi.org/10.1093/mnras/stac258
Comments
This article originally appeared in Monthly Notices of the Royal Astronomical Society, Volume 511, Issue 3, 2022. The article can also be found online at: https://doi.org/10.1093/mnras/stac258.