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dc.contributor.authorRyder, S.D.
dc.contributor.authorSharp, R.G.
dc.contributor.authorKnapen, J.
dc.contributor.authorMazzuca, L.M.
dc.contributor.authorParry, I.R.
dc.date.accessioned2012-08-06T09:01:52Z
dc.date.available2012-08-06T09:01:52Z
dc.date.issued2005
dc.identifier.citationRyder , S D , Sharp , R G , Knapen , J , Mazzuca , L M & Parry , I R 2005 , The Circumnuclear Starburst in M83 . in The evolution of starbursts : the 331st Wilhelm & Else Heraeus Seminar . AIP Conf Procs , vol. 783 , American Institute of Physics (AIP) , pp. 155-160 , The evolution of starbursts: the 331st Wilhelm & Else Heraeus Seminar , Bad Honnef , Germany , 16/08/04 . https://doi.org/10.1063/1.2034980
dc.identifier.citationconference
dc.identifier.otherPURE: 968793
dc.identifier.otherPURE UUID: fc4f8eeb-1db9-4787-9ccb-8946f6a5488e
dc.identifier.otherdspace: 2299/3693
dc.identifier.otherScopus: 33749578380
dc.identifier.urihttp://hdl.handle.net/2299/8787
dc.descriptionOriginal paper can be found at http://www.virtualjournals.org/proceedings/confproceed/783.jsp Copyright American Institute of Physics. DOI: 10.1063/1.2034980 [Full text of this article is not available in the UHRA]
dc.description.abstractWe present results from near-infrared integral-field spectroscopy of the circumnuclear starburst in M83, using the CIRPASS instrument on Gemini South. The combination of Pa, CO (6,3), and [Fe II] equivalent width measurements over large contiguous regions allows us to track the spatial propagation of star formation across the ringlet, which is too heavily obscured to be properly analysed at optical wavelengths. We find the clearest evidence yet for an age gradient, with the youngest clusters found closest to where the dust lane crosses the ringlet. We discuss the implications for gas fueling by the bar.en
dc.language.isoeng
dc.publisherAmerican Institute of Physics (AIP)
dc.relation.ispartofThe evolution of starbursts
dc.relation.ispartofseriesAIP Conf Procs
dc.titleThe Circumnuclear Starburst in M83en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
rioxxterms.versionofrecordhttps://doi.org/10.1063/1.2034980
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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