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dc.contributor.authorRyder, S.D.
dc.contributor.authorKnapen, J.
dc.date.accessioned2009-07-22T13:20:45Z
dc.date.available2009-07-22T13:20:45Z
dc.date.issued2001
dc.identifier.citationRyder , S D & Knapen , J 2001 , ' Circumnuclear Star Formation in M100 ' , Astrophysics and Space Science , vol. 276 , no. 2/4 , pp. 405-412 . https://doi.org/10.1023/A:1017578713184
dc.identifier.issn0004-640X
dc.identifier.otherPURE: 156546
dc.identifier.otherPURE UUID: 496fd9b7-4030-435a-ab6a-755088350714
dc.identifier.otherdspace: 2299/3701
dc.identifier.otherScopus: 0035647962
dc.identifier.urihttp://hdl.handle.net/2299/3701
dc.description“The original publication is available at www.springerlink.com”. Copyright Springer. [Full text of this article is not available in the UHRA]
dc.description.abstractNear-infrared (JHK) images of the nucleus of the barred spiral galaxy M100 (NGC 4321) have been obtained using a high-bandwidth tip-tilt secondary and fast guider system on the 3.8 m United Kingdom Infrared Telescope (UKIRT). The resulting images, with a resolution of 0.34″ at K, reveal for the first time a host of compact ‘knots’, which appear to be the result of a recent burst (or bursts) of star formation. Confirmation of this comes from K-band spectroscopy of these knots with CGS4 on UKIRT, which shows Brγ emission and CO absorption features. A comparison with starburst evolutionary models suggests ages for these knots of between 17 and 27 Myr, and a stellar population dominated by late-type supergiants.en
dc.language.isoeng
dc.relation.ispartofAstrophysics and Space Science
dc.titleCircumnuclear Star Formation in M100en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2001
rioxxterms.versionofrecordhttps://doi.org/10.1023/A:1017578713184
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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