dc.contributor.author Chen, Hao dc.contributor.author Sun, Ming dc.contributor.author Yagi, Masafumi dc.contributor.author Bravo-Alfaro, Hector dc.contributor.author Brinks, Elias dc.contributor.author Kenney, Jeffrey dc.contributor.author Combes, Francoise dc.contributor.author Sivanandam, Suresh dc.contributor.author Jachym, Pavel dc.contributor.author Fossati, Matteo dc.contributor.author Gavazzi, Giuseppe dc.contributor.author Boselli, Alessandro dc.contributor.author Nulsen, Paul dc.contributor.author Sarazin, Craig dc.contributor.author Ge, Chong dc.contributor.author Yoshida, Michitoshi dc.contributor.author Roediger, Elke dc.date.accessioned 2020-07-26T00:25:37Z dc.date.available 2020-07-26T00:25:37Z dc.date.issued 2020-08 dc.identifier.citation Chen , H , Sun , M , Yagi , M , Bravo-Alfaro , H , Brinks , E , Kenney , J , Combes , F , Sivanandam , S , Jachym , P , Fossati , M , Gavazzi , G , Boselli , A , Nulsen , P , Sarazin , C , Ge , C , Yoshida , M & Roediger , E 2020 , ' The ram pressure stripped radio tails of galaxies in the Coma cluster ' , Monthly Notices of the Royal Astronomical Society , vol. 496 , no. 4 , pp. 4654–4673 . https://doi.org/10.1093/mnras/staa1868 dc.identifier.issn 0035-8711 dc.identifier.other PURE: 22220573 dc.identifier.other PURE UUID: e71af8d4-3e80-4163-a3f5-bac8f3ae41e7 dc.identifier.other ArXiv: http://arxiv.org/abs/2004.06743v2 dc.identifier.other ORCID: /0000-0002-7758-9699/work/77850103 dc.identifier.other Scopus: 85091468496 dc.identifier.uri http://hdl.handle.net/2299/22998 dc.description This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, Volume 496, Issue 4, August 2020, Pages 4654–4673, https://doi.org/10.1093/mnras/staa1868. ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. dc.description.abstract Previous studies have revealed a population of galaxies in galaxy clusters with ram pressure stripped (RPS) tails of gas and embedded young stars. We observed 1.4 GHz continuum and HI emission with the Very Large Array in its B-configuration in two fields of the Coma cluster to study the radio properties of RPS galaxies. The best continuum sensitivities in the two fields are 6 and 8 $\mu$Jy per 4'' beam respectively, which are 4 and 3 times deeper than those previously published. Radio continuum tails are found in 10 (8 are new) out of 20 RPS galaxies, unambiguously revealing the presence of relativistic electrons and magnetic fields in the stripped tails. Our results also hint that the tail has a steeper spectrum than the galaxy. The 1.4 GHz continuum in the tails is enhanced relative to their H$\alpha$ emission by a factor of $\sim$7 compared to the main bodies of the RPS galaxies. The 1.4 GHz continuum of the RPS galaxies is also enhanced relative to their IR emission by a factor of $\sim$2 compared to star-forming galaxies. The enhancement is likely related to ram pressure and turbulence in the tail. We furthermore present HI detections in three RPS galaxies and upper limits for the other RPS galaxies. The cold gas in D100's stripped tail is dominated by molecular gas, which is likely a consequence of the high ambient pressure. No evidence of radio emission associated with ultra-diffuse galaxies is found in our data. en dc.format.extent 20 dc.language.iso eng dc.relation.ispartof Monthly Notices of the Royal Astronomical Society dc.rights Open dc.subject astro-ph.GA dc.title The ram pressure stripped radio tails of galaxies in the Coma cluster en dc.contributor.institution Centre for Astrophysics Research dc.contributor.institution School of Physics, Astronomy and Mathematics dc.contributor.institution School of Physics, Engineering & Computer Science dc.contributor.institution Department of Physics, Astronomy and Mathematics dc.description.status Peer reviewed dc.relation.school School of Physics, Engineering & Computer Science dc.description.versiontype Final Published version dcterms.dateAccepted 2020-08 rioxxterms.version VoR rioxxterms.versionofrecord https://doi.org/10.1093/mnras/staa1868 rioxxterms.licenseref.uri Unspecified rioxxterms.type Journal Article/Review herts.preservation.rarelyaccessed true herts.rights.accesstype Open
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