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dc.contributor.authorWestcott, Jonathan
dc.contributor.authorBrinks, Elias
dc.contributor.authorBeswick, R. J.
dc.contributor.authorHeesen, V.
dc.contributor.authorArgo, M. K.
dc.contributor.authorBaldi, R. D.
dc.contributor.authorFenech, D. M.
dc.contributor.authorMcHardy, I. M.
dc.contributor.authorSmith, Daniel
dc.contributor.authorWilliams, D. R. A.
dc.date.accessioned2018-08-16T00:10:49Z
dc.date.available2018-08-16T00:10:49Z
dc.date.issued2017-01-22
dc.identifier.citationWestcott , J , Brinks , E , Beswick , R J , Heesen , V , Argo , M K , Baldi , R D , Fenech , D M , McHardy , I M , Smith , D & Williams , D R A 2017 , ' A High-Resolution Radio Continuum Study Of The Dwarf Irregular Galaxy IC 10 ' , Monthly Notices of the Royal Astronomical Society . https://doi.org/10.1093/mnras/stx188
dc.identifier.issn1365-2966
dc.identifier.otherPURE: 11099670
dc.identifier.otherPURE UUID: 485819df-4534-49fd-bedb-aca311c03c3e
dc.identifier.otherArXiv: http://arxiv.org/abs/1701.06571v1
dc.identifier.otherScopus: 85018364139
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407784
dc.identifier.otherORCID: /0000-0001-9708-253X/work/69424311
dc.identifier.urihttp://hdl.handle.net/2299/20359
dc.descriptionThis is the accepted manuscript version of an article accepted for publication in Monthly Notices of the Royal Astronomical Society. J. Westcott et al, A High-Resolution Radio Continuum Study Of The Dwarf Irregular Galaxy IC 10, MNRAS 000, 1-15 (2016). Preprint 22 January 2017, doi: https://doi.org/10.1093/mnras/stx188 © 2017 The Authors
dc.description.abstractWe present high-resolution e-MERLIN radio continuum maps of the Dwarf Irregular galaxy IC10 at 1.5GHz and 5GHz. We detect 11 compact sources at 1.5GHz, 5 of which have complementary detections at 5GHz. We classify 3 extended sources as compact H{\sc ii} regions within IC10, 5 sources as contaminating background galaxies and identify 3 sources which require additional observations to classify. We do not expect that any of these 3 sources are Supernova Remnants as they will likely be resolved out at the assumed distance of IC10 (0.7Mpc). We correct integrated flux densities of IC10 from the literature for contamination by unrelated background sources and obtain updated flux density measurements of $354\pm11$\,mJy at 1.5GHz and $199\pm9$\,mJy at 4.85GHz. The background contamination does not contribute significantly to the overall radio emission from IC10, so previous analysis concerning its integrated radio properties remain valid.en
dc.format.extent15
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsOpen
dc.subjectastro-ph.GA
dc.subjectgalaxies: dwarf
dc.subjectgalaxies: ISM
dc.subjectISM: supernova remnants
dc.subjectISM: HII regions
dc.subjecttechniques: high angular resolution
dc.subjecttechniques: interferometric
dc.titleA High-Resolution Radio Continuum Study Of The Dwarf Irregular Galaxy IC 10en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttps://arxiv.org/pdf/1701.06571v1.pdf
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2017-01-22
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stx188
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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