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EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey
M. G. Guarcello, E. Flaccomio, J. F. Albacete-Colombo +48
Context. With a mass exceeding several 10^4 solar masses and a rich and dense population of massive stars, supermassive young star clusters represent the most massive star-forming…
A closer look at the binary content of NGC 1850
S. Saracino, S. Kamann, N. Bastian +7
Studies of young clusters have shown that a large fraction of O-/early B-type stars are in binary systems, where the binary fraction increases with mass. These massive stars are pr…
Updated radial velocities and new constraints on the nature of the unseen source in NGC1850 BH1
Sara Saracino, Tomer Shenar, Sebastian Kamann +7
A black hole candidate orbiting a luminous star in the Large Magellanic Cloud young cluster NGC 1850 (Myr) has recently been reported based on radial velocity and light cu…
On the origin of UV-dim stars: a population of rapidly rotating shell stars?
Silvia Martocchia, Nate Bastian, Sara Saracino +1
The importance of stellar rotation in setting the observed properties of young star clusters has become clearer over the past decade, with rotation being identified as the main cau…
In-situ or accreted? Using deep learning to infer the origin of extragalactic globular clusters from observables
Sebastian Trujillo-Gomez, J. M. Diederik Kruijssen, Joel Pfeffer +4
Globular clusters (GCs) are powerful tracers of the galaxy assembly process, and have already been used to obtain a detailed picture of the progenitors of the Milky Way. Using the…