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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Dettagli Bibliografici
Autori principali:	Kuvatova, D., Ishchenko, M., Berczik, P., Veles, O., Sobodar, O., Panamarev, T.
Natura:	Preprint
Pubblicazione:	2026
Soggetti:	Astrophysics of Galaxies
Accesso online:	Acceder al recurso
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