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Multiple Stellar Populations in Globular Clusters
Nate Bastian, Carmela Lardo
Globular Clusters (GCs) exhibit star-to-star variations in specific elements (e.g., He, C, N, O, Na, Al) that bare the hallmark of high temperature H burning. These abundance varia…
The E-MOSAICS Project: simulating the formation and co-evolution of galaxies and their star cluster populations
Joel Pfeffer, J. M. Diederik Kruijssen, Robert A. Crain +1
We introduce the MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE (E-MOSAICS) project. E-MOSAICS incorporates models describing the formation, ev…
Interpreting the complex CMDs of the Magellanic Clouds clusters
I. Cabrera-Ziri, S. Martocchia, K. Hollyhead +1
The Magellanic Clouds host a large population of massive (> 10^4 Msun) star clusters with ages ranging from a few Myr to 12 Gyr. In nearly all cases, close inspection of their CMDs…
Nearby Early-Type Galactic Nuclei at High Resolution: Dynamical Black Hole and Nuclear Star Cluster Mass Measurements
Dieu D. Nguyen, Anil C. Seth, Nadine Neumayer +12
We present a detailed study of the nuclear star clusters (NSCs) and massive black holes (BHs) of four of the nearest low-mass early-type galaxies: M32, NGC205, NGC5012, and NGC5206…
The VLT-FLAMES Tarantula Survey
Jorick S. Vink, C. J. Evans, J. Bestenlehner +5
We present a number of notable results from the VLT-FLAMES Tarantula Survey (VFTS), an ESO Large Program during which we obtained multi-epoch medium-resolution optical spectroscopy…
Age as a Major Factor in the Onset of Multiple Populations in Stellar Clusters
S. Martocchia, I. Cabrera-Ziri, C. Lardo +16
It is now well established that globular clusters (GCs) exhibit star-to-star light-element abundance variations (known as multiple stellar populations, MPs). Such chemical anomalie…