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DTSTART;TZID=Europe/Rome:20231113T113000
DTEND;TZID=Europe/Rome:20231113T123000
DTSTAMP:20260407T031741
CREATED:20231027T042658Z
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UID:12389-1699875000-1699878600@www.oa-roma.inaf.it
SUMMARY:colloquium - Richard de Grijs: Unveiling the complexities of massive star clusters
DESCRIPTION:Around the turn of the last century\, star clusters of all kinds were considered ‘simple’ stellar populations. Over the past decades\, this situation has changed dramatically. At the same time\, star clusters are among the brightest stellar population components and\, as such\, they are visible out to much greater distances than individual stars\, even the brightest\, so that understanding the intricacies of star cluster composition and their evolution is imperative for understanding stellar populations and the evolution of galaxies as a whole. In this brief review of where the field has moved to in recent years\, we place particular emphasis on the properties and importance of the effects of rapid stellar rotation\, and the presence of multiplicity among the red-giant-branch populations in Magellanic Cloud star clusters with ages up to a few billion years.
URL:https://www.oa-roma.inaf.it/event/colloqium-richard-de-grijs-unveiling-the-complexities-of-massive-star-clusters/
LOCATION:Aula Gratton
CATEGORIES:Seminari
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