The young massive SMC cluster NGC 330 seen by MUSE III. Stellar parameters and rotational velocities

Bodensteiner, J.; Sana, H.; Dufton, P. L.; Wang, C.; Langer, N.; Banyard, G.; Mahy, L.; de Koter, A.; de Mink, S. E.; Evans, C. J.; Gotberg, Y.; Henault-Brunet, V.; Patrick, L. R.; Schneider, F. R. N.
2023
ASTRONOMY & ASTROPHYSICS
DOI
10.1051/0004-6361/202345950
Context. The origin of the initial rotation rates of stars, and how a star's surface rotational velocity changes during the evolution, either by internal angular momentum transport or due to interactions with a binary companion, remain open questions in stellar astrophysics.