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dc.contributor.authorKnapen, J.
dc.contributor.authorStedman, S.
dc.date.accessioned2008-01-30T10:38:12Z
dc.date.available2008-01-30T10:38:12Z
dc.date.issued2002
dc.identifier.citationKnapen , J & Stedman , S 2002 , An Imaging survey of nearby spiral galaxies . in In: Procs of Disks of Galaxies: Kinematics, Dynamics and Peturbations - ASP Conference Series 275 . Astronomical Society of the Pacific , pp. 319-322 .
dc.identifier.isbn1-58381-117-6
dc.identifier.otherPURE: 144969
dc.identifier.otherPURE UUID: afc33a39-05e2-4871-b461-ec2d6f2ccbd9
dc.identifier.otherdspace: 2299/1455
dc.identifier.urihttp://hdl.handle.net/2299/1455
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/253.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe describe the progress of a large optical and near-infrared imaging study of a complete sample of 57 spiral galaxies. We have obtained B, I, K' and Ha imaging to map stellar populations and massive star formation (SF) across the arm and interarm regions, in order to study the distribution of mass and SF in these different and distinct environments. We briefly describe the background to our program, the sample selection,observations, and the reduction procedures. We present a K' image and preliminary radial profiles of the SABcd (SXT6) galaxy NGC 1042. SF appears to induce differences between the arm and interarm profiles, and to enlarge the scale length of the exponential disk of the galaxy.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Disks of Galaxies: Kinematics, Dynamics and Peturbations - ASP Conference Series 275
dc.rightsOpen
dc.titleAn Imaging survey of nearby spiral galaxiesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2002
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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