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SKA studies of nearby galaxies : star-formation, accretion processes and molecular gas across all environments

dc.contributor.authorBeswick, R. J.
dc.contributor.authorBrinks, E.
dc.contributor.authorPerez-Torres, M. A.
dc.contributor.authorRichards, A. M. S.
dc.contributor.authorAalto, S.
dc.contributor.authorAlberdi, A.
dc.contributor.authorArgo, M.K.
dc.contributor.authorBemmel, I. van
dc.contributor.authorConway, J. E.
dc.contributor.authorDickinson, C.
dc.contributor.authorFenech, D. M.
dc.contributor.authorGray, M.D.
dc.contributor.authorKlockner, H-R
dc.contributor.authorMurphy, E. J.
dc.contributor.authorMuxlow, T.W.B.
dc.contributor.authorPeel, M.
dc.contributor.authorRushton, A. P.
dc.contributor.authorSchinnerer, E.
dc.date.accessioned2015-06-02T11:21:06Z
dc.date.available2015-06-02T11:21:06Z
dc.date.issued2015-05-29
dc.identifier.citationBeswick , R J , Brinks , E , Perez-Torres , M A , Richards , A M S , Aalto , S , Alberdi , A , Argo , M K , Bemmel , I V , Conway , J E , Dickinson , C , Fenech , D M , Gray , M D , Klockner , H-R , Murphy , E J , Muxlow , T W B , Peel , M , Rushton , A P & Schinnerer , E 2015 , ' SKA studies of nearby galaxies : star-formation, accretion processes and molecular gas across all environments ' , Proceedings of Science , vol. 215 , 070 . https://doi.org/10.22323/1.215.0070
dc.identifier.issn1824-8039
dc.identifier.otherArXiv: http://arxiv.org/abs/1412.5810v1
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407798
dc.identifier.urihttp://hdl.handle.net/2299/15986
dc.descriptionCopyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence
dc.description.abstractThe SKA will be a transformational instrument in the study of our local Universe. In particular, by virtue of its high sensitivity (both to point sources and diffuse low surface brightness emission), angular resolution and the frequency ranges covered, the SKA will undertake a very wide range of astrophysical research in the field of nearby galaxies. By surveying vast numbers of nearby galaxies of all types with $\mu$Jy sensitivity and sub-arcsecond angular resolutions at radio wavelengths, the SKA will provide the cornerstone of our understanding of star-formation and accretion activity in the local Universe. In this chapter we outline the key continuum and molecular line science areas where the SKA, both during phase-1 and when it becomes the full SKA, will have a significant scientific impact.en
dc.format.extent23
dc.format.extent5194279
dc.language.isoeng
dc.relation.ispartofProceedings of Science
dc.subjectastro-ph.GA
dc.subjectastro-ph.CO
dc.titleSKA studies of nearby galaxies : star-formation, accretion processes and molecular gas across all environmentsen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
dc.identifier.urlhttp://pos.sissa.it/archive/conferences/215/070/AASKA14_070.pdf
rioxxterms.versionofrecord10.22323/1.215.0070
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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