How our proto-nuclear star cluster formed and grew due to early globular cluster disruption. I. Case of low masses

Fuente: arXiv

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Bibliographic Details
Main Authors:	Kuvatova, D., Ishchenko, M., Berczik, P., Veles, O., Sobodar, O., Panamarev, T.
Format:	Preprint
Published:	2026
Subjects:	Astrophysics of Galaxies
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2601.01867