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From the top down and back up again: star cluster structure from hierarchical star formation
Young massive star clusters spanning ~10(4)–10(8)M(⊙) in mass have been observed to have similar surface brightness profiles. We show that recent hydrodynamical simulations of star cluster formation have also produced star clusters with this structure. We argue analytically that this type of mass di...
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| Publicado no: | Mon Not R Astron Soc |
|---|---|
| Main Authors: | , , , , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
2018
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6296242/ https://ncbi.nlm.nih.gov/pubmed/30573926 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1093/mnras/sty2303 |
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