Show simple item record

dc.contributor.authorAnders, P.
dc.contributor.authorFritze, U.
dc.contributor.authorde Grijs, R.
dc.date.accessioned2009-12-04T10:15:19Z
dc.date.available2009-12-04T10:15:19Z
dc.date.issued2009
dc.identifier.citationAnders , P , Fritze , U & de Grijs , R 2009 , ' The young star cluster system of the Antennae galaxies ' , Astrophysics and Space Science , vol. 324 , no. 2-4 , pp. 305-308 . https://doi.org/10.1007/s10509-009-0103-x
dc.identifier.issn0004-640X
dc.identifier.otherPURE: 156049
dc.identifier.otherPURE UUID: 6805504a-476b-44be-93d5-d31018f0af93
dc.identifier.otherdspace: 2299/4057
dc.identifier.otherScopus: 84895900789
dc.identifier.urihttp://hdl.handle.net/2299/4057
dc.description“The original publication is available at www.springerlink.com”. Copyright Springer. DOI: 10.1007/s10509-009-0103-x
dc.description.abstractThe study of young star cluster (YSC) systems, preferentially in starburst and merging galaxies, has seen great interest in the recent past, as it provides important input to models of star formation. However, even some basic properties (such as the luminosity function; LF) of YSC systems are still being debated. Here, we study the photometric properties of the YSC system in the nearest major merger system, the Antennae galaxies. We find evidence for the existence of a statistically significant turnover in the LF.en
dc.language.isoeng
dc.relation.ispartofAstrophysics and Space Science
dc.titleThe young star cluster system of the Antennae galaxiesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1007/s10509-009-0103-x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record