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dc.contributor.authorBaldi, R. D.
dc.contributor.authorWilliams, D. R. A.
dc.contributor.authorMcHardy, I. M.
dc.contributor.authorBeswick, R. J.
dc.contributor.authorBrinks, E.
dc.contributor.authorDullo, B. T.
dc.contributor.authorKnapen, J. H.
dc.contributor.authorArgo, M. K.
dc.contributor.authorAalto, S.
dc.contributor.authorAlberdi, A.
dc.contributor.authorBaan, W. A.
dc.contributor.authorBendo, G. J.
dc.contributor.authorCorbel, S.
dc.contributor.authorFenech, D. M.
dc.contributor.authorGallagher, J. S.
dc.contributor.authorGreen, D. A.
dc.contributor.authorKennicutt, R. C.
dc.contributor.authorKlöckner, H. -R.
dc.contributor.authorKörding, E.
dc.contributor.authorMaccarone, T. J.
dc.contributor.authorMuxlow, T. W. B.
dc.contributor.authorMundell, C. G.
dc.contributor.authorPanessa, F.
dc.contributor.authorPeck, A. B.
dc.contributor.authorPérez-Torres, M. A.
dc.contributor.authorRomero-Cañizales, C.
dc.contributor.authorSaikia, P.
dc.contributor.authorShankar, F.
dc.contributor.authorSpencer, R. E.
dc.contributor.authorStevens, I. R.
dc.contributor.authorVarenius, E.
dc.contributor.authorWard, M. J.
dc.contributor.authorYates, J.
dc.date.accessioned2020-11-18T14:15:03Z
dc.date.available2020-11-18T14:15:03Z
dc.date.issued2020-11-17
dc.identifier.citationBaldi , R D , Williams , D R A , McHardy , I M , Beswick , R J , Brinks , E , Dullo , B T , Knapen , J H , Argo , M K , Aalto , S , Alberdi , A , Baan , W A , Bendo , G J , Corbel , S , Fenech , D M , Gallagher , J S , Green , D A , Kennicutt , R C , Klöckner , H -R , Körding , E , Maccarone , T J , Muxlow , T W B , Mundell , C G , Panessa , F , Peck , A B , Pérez-Torres , M A , Romero-Cañizales , C , Saikia , P , Shankar , F , Spencer , R E , Stevens , I R , Varenius , E , Ward , M J & Yates , J 2020 , ' LeMMINGs. II. The e-MERLIN legacy survey of nearby galaxies. The deepest radio view of the Palomar sample on parsec scale ' , Monthly Notices of the Royal Astronomical Society . https://doi.org/10.1093/mnras/staa3519
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 22964677
dc.identifier.otherPURE UUID: 5640ee4b-5c88-4995-8e9b-08d9817fb678
dc.identifier.otherArXiv: http://arxiv.org/abs/2011.03062v1
dc.identifier.otherORCID: /0000-0002-7758-9699/work/83844935
dc.identifier.otherScopus: 85099682315
dc.identifier.urihttp://hdl.handle.net/2299/23474
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
dc.description.abstractWe present the second data release of high-resolution ($\leq0.2$ arcsec) 1.5-GHz radio images of 177 nearby galaxies from the Palomar sample, observed with the e-MERLIN array, as part of the LeMMINGs (Legacy e-MERLIN Multi-band Imaging of Nearby Galaxy Sample) survey. Together with the 103 targets of the first LeMMINGs data release, this represents a complete sample of 280 local active (LINER and Seyfert) and inactive galaxies HII galaxies and Absorption Line Galaxies, ALG). This large program is the deepest radio survey of the local Universe, $\gtrsim$10$^{17.6}$ W Hz$^{-1}$, regardless of the host and nuclear type: we detect radio emission $\gtrsim$0.25 mJy beam$^{-1}$ for 125/280 galaxies (44.6 per cent) with sizes of typically $\lesssim$100 pc. Of those 125, 106 targets show a core which coincides within 1.2 arcsec with the optical nucleus. Although we observed mostly cores, around one third of the detected galaxies features jetted morphologies. The detected radio core luminosities of the sample range between $\sim$10$^{34}$ and 10$^{40}$ erg s$^{-1}$. LINERs and Seyferts are the most luminous sources, whereas HII galaxies are the least. LINERs show FRI-like core-brightened radio structures, while Seyferts reveal the highest fraction of symmetric morphologies. The majority of HII galaxies have single radio core or complex extended structures, which probably conceal a nuclear starburst and/or a weak active nucleus (seven of them show clear jets). ALGs, which are typically found in evolved ellipticals, although the least numerous, exhibit on average the most luminous radio structures, similar to LINERs.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsOpen
dc.subjectastro-ph.GA
dc.subjectastro-ph.HE
dc.titleLeMMINGs. II. The e-MERLIN legacy survey of nearby galaxies. The deepest radio view of the Palomar sample on parsec scaleen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Engineering & Computer Science
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2020-11-17
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/staa3519
rioxxterms.licenseref.uriOther
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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