Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource Articles Article Faculty Publications -Articles Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource GASP XVIII: Star formation quenching due to AGN feedback in the central region of a jellyfish galaxy Subject The topic of the resource galaxies: clusters: intracluster medium; galaxies: star formation Description An account of the resource We report evidence for star formation quenching in the central 8.6 kpc region of the jellyfish galaxy JO201 that hosts an active galactic nucleus (AGN), while undergoing strong ram-pressure stripping. The ultraviolet imaging data of the galaxy disc reveal a region with reduced flux around the centre of the galaxy and a horse-shoe-shaped region with enhanced flux in the outer disc. The characterization of the ionization regions based on emission line diagnostic diagrams shows that the region of reduced flux seen in the ultraviolet is within the AGN-dominated area. The CO J2-1 map of the galaxy disc reveals a cavity in the central region. The image of the galaxy disc at redder wavelengths (9050-9250 reveals the presence of a stellar bar. The star formation rate map of the galaxy disc shows that the star formation suppression in the cavity occurred in the last few 108 yr. We present several lines of evidence supporting the scenario that suppression of star formation in the central region of the disc is most likely due to the feedback from the AGN. The observations reported here make JO201 a unique case of AGN feedback and environmental effects suppressing star formation in a spiral galaxy. 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. Creator An entity primarily responsible for making the resource George K.; Poggianti B.M.; Bellhouse C.; Radovich M.; Fritz J.; Paladino R.; Bettoni D.; JaffY.; Moretti A.; Gullieuszik M.; Vulcani B.; Fasano G.; Stalin C.S.; Subramaniam A.; Tandon S.N. Source A related resource from which the described resource is derived Monthly Notices of the Royal Astronomical Society, Vol-487, No. 3, pp. 3102-3111. Publisher An entity responsible for making the resource available Oxford University Press Date A point or period of time associated with an event in the lifecycle of the resource 2019-01-01 Identifier An unambiguous reference to the resource within a given context <a href="https://doi.org/10.1093/mnras/stz1443" target="_blank" rel="noreferrer noopener">https://doi.org/10.1093/mnras/stz1443</a> <br /><br /><a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85072295444&amp;doi=10.1093%2Fmnras%2Fstz1443&amp;partnerID=40&amp;md5=47f7d49a9aa806f59b58c46c050d00e8" target="_blank" rel="noreferrer noopener">https://www.scopus.com/inward/record.uri?eid=2-s2.0-85072295444&amp;doi=10.1093%2fmnras%2fstz1443&amp;partnerID=40&amp;md5=47f7d49a9aa806f59b58c46c050d00e8</a> Rights Information about rights held in and over the resource All Open Access; Green Open Access Relation A related resource ISSN: 358711; CODEN: MNRAA Format The file format, physical medium, or dimensions of the resource Online Language A language of the resource English Type The nature or genre of the resource Article Coverage The spatial or temporal topic of the resource, the spatial applicability of the resource, or the jurisdiction under which the resource is relevant George K., Indian Institute of Astrophysics, Koramangala II Block, Bangalore, 560034, India, Department of Physics, Christ University, Hosur Road, Bangalore, 560029, India; Poggianti B.M., INAF-Astronomical Observatory of Padova, vicolo dell'Osservatorio 5, Padova, I-35122, Italy; Bellhouse C., School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, United Kingdom; Radovich M., INAF-Astronomical Observatory of Padova, vicolo dell'Osservatorio 5, Padova, I-35122, Italy; Fritz J., Instituto de Radioastronomia y Astrofisica, UNAM, Campus Morelia, A.P. 3-72, C.P., Morelia, 58089, Mexico; Paladino R., Instituto Nazionale di Astrofisica - Istituto di Radioastronomia, Via P. Gobetti 101, Bologna, I-40129, Italy; Bettoni D., INAF-Astronomical Observatory of Padova, vicolo dell'Osservatorio 5, Padova, I-35122, Italy; JaffY., Instituto de Ficay Astronom, Universidad de Valparaiso, Gran Breta 1111, Valparaiso, Chile; Moretti A., INAF-Astronomical Observatory of Padova, vicolo dell'Osservatorio 5, Padova, I-35122, Italy; Gullieuszik M., INAF-Astronomical Observatory of Padova, vicolo dell'Osservatorio 5, Padova, I-35122, Italy; Vulcani B., INAF-Astronomical Observatory of Padova, vicolo dell'Osservatorio 5, Padova, I-35122, Italy; Fasano G., INAF-Astronomical Observatory of Padova, vicolo dell'Osservatorio 5, Padova, I-35122, Italy; Stalin C.S., Indian Institute of Astrophysics, Koramangala II Block, Bangalore, 560034, India; Subramaniam A., Indian Institute of Astrophysics, Koramangala II Block, Bangalore, 560034, India; Tandon S.N., Indian Institute of Astrophysics, Koramangala II Block, Bangalore, 560034, India, Inter-University Center for Astronomy and Astrophysics, Pune, India