{"paper":{"title":"Unveiling the 100 pc scale nuclear radio structure of NGC 6217 with e-MERLIN and the VLA","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(10) Cavendish Laboratory, (11) National Centre for Radio Astrophysics - Tata Institute of Fundamental Research, 12), (12) Liverpool John Moores University), 2), (2) Department of Physics, (3) Jodrell Bank Centre for Astrophysics, 4), (4) University of Central Lancashire, 5), (5) DST-INSPIRE Faculty, (6) Centre for Astrophysics Research, (7) Departamento de Astrofisica y Ciencias de la Atmosfera, 8, (8) Instituto de Astrofisica de Canarias, 9, 9), (9) Departamento de Astrofisica, Aru Beri (1, Astronomy, Bililign T. Dullo (7, Danielle M. Fenech (10), David R. A. Williams (1, Elias Brinks (6), Ian M. McHardy (1), IISER, Jeremiah Horrocks Institute, Johan H. Knapen (8, Jonathan Westcott (6) ((1) School of Physics, Judith Ineson (1), Mayukh Pahari (1), Megan K. Argo (3, Peter Boorman (1), Preeti Kharb (11), Ranieri D. Baldi (1), Robert J. Beswick (3), School of Physics, The University of Manchester, Tom W. B. Muxlow (3), Universidad Complutense de Madrid, Universidad de La Laguna, University of Cambridge, University of Hertfordshire, University of Oxford, University of Southampton","submitted_at":"2019-04-23T11:48:51Z","abstract_excerpt":"We present high-sensitivity 1.51 GHz e-MERLIN radio images of the nearby galaxy NGC 6217. We resolve the compact radio source at the centre of NGC 6217 for the first time, finding a twin-lobed structure with a total linear size of ~4 arcsec (~400pc). The radio source does not have a compact central core but there is an unresolved hot spot near the outer edge of the southern lobe. Combining our e-MERLIN data with new VLA A-Array data and archival multi-wavelength data, we explore possible scenarios which might explain this complex radio morphology. We conclude that this radio source is most lik"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.10259","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}