Stirred, not shaken: star cluster survival in the slingshot scenario

We investigate the effects of an oscillating gas filament on the dynamics of its embedded stellar clusters. Motivated by recent observational constraints, we model the host gas filament as a cylindrically symmetrical potential, and the star cluster as a Plummer sphere. In the model, the motion of th...

Täydet tiedot

Bibliografiset tiedot
Päätekijät: Carrillo, DRM, Fellhauer, M, Boekholt, TCN, Stutz, A, Inostroza, MCBM
Aineistotyyppi: Journal article
Kieli:English
Julkaistu: Oxford University Press 2023