English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/237371
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE
Exportar a otros formatos:


Star clusters near and far

Other TitlesTracing star formation across cosmic time
AuthorsAdamo, Angela; Zeidler, Peter; Diederik Kruijssen, J. M.; Chevance, Mélanie; Gieles, Mark; Calzetti, Daniela; Charbonnel, Corinne; Zinnecker, Hans; Krause, Martin G. H.
Issue Date2020
PublisherSpringer Nature
CitationSpace Science Reviews 216: 69 (2020)
AbstractStar clusters are fundamental units of stellar feedback and unique tracers of their host galactic properties. In this review, we will first focus on their constituents, i.e. detailed insight into their stellar populations and their surrounding ionised, warm, neutral, and molecular gas. We, then, move beyond the Local Group to review star cluster populations at various evolutionary stages, and in diverse galactic environmental conditions accessible in the local Universe. At high redshift, where conditions for cluster formation and evolution are more extreme, we are only able to observe the integrated light of a handful of objects that we believe will become globular clusters. We therefore discuss how numerical and analytical methods, informed by the observed properties of cluster populations in the local Universe, are used to develop sophisticated simulations potentially capable of disentangling the genetic map of galaxy formation and assembly that is carried by globular cluster populations.
Publisher version (URL)https://doi.org/10.1007/s11214-020-00690-x
Appears in Collections:(ICE) Artículos
Files in This Item:
File Description SizeFormat 
starfar.pdf4,06 MBAdobe PDFThumbnail
Show full item record
Review this work

Related articles:

WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.