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dc.rights.licenseCopyright © 2021, The Author(s), under exclusive licence to Springer Nature Limited-
dc.contributor.authorPuglisi, A.-
dc.contributor.authorDaddi, E.-
dc.contributor.authorBrusa, M.-
dc.contributor.authorBournaud, F.-
dc.contributor.authorFensch, J.-
dc.contributor.authorLiu, D.-
dc.contributor.authorDelvecchio, I.-
dc.contributor.authorCalabrò, A.-
dc.contributor.authorCircosta, C.-
dc.contributor.authorValentino, F.-
dc.contributor.authorPerna, M.-
dc.contributor.authorJin, S.-
dc.contributor.authorEnia, A.-
dc.contributor.authorMancini, C.-
dc.contributor.authorRodighiero, G.-
dc.date.accessioned2022-02-14T10:37:25Z-
dc.date.available2022-02-14T10:37:25Z-
dc.date.issued2021-01-11-
dc.identifier.citationNature Astronomy 5: 319-330(2021)es
dc.identifier.urihttp://hdl.handle.net/20.500.12666/540-
dc.descriptionThe ALMA data analysed in this study are publicly available from the ALMA archive (http://almascience.nrao.edu/aq/, Program IDs: 2015.1.00260.S, 2016.1.00171.S and 2019.1.01702.S). The DEIMOS spectrum of the source is also publicly available and can be retrieved through the COSMOS archive (http://cosmos.astro.caltech.edu/).es
dc.description.abstractFeedback-driven winds from star formation or active galactic nuclei might be a relevant channel for the abrupt quenching of star formation in massive galaxies. However, both observations and simulations support the idea that these processes are non-conflictingly co-evolving and self-regulating. Furthermore, evidence of disruptive events that are capable of fast quenching is rare, and constraints on their statistical prevalence are lacking. Here we present a massive starburst galaxy at redshift z = 1.4, which is ejecting 46 ± 13% of its molecular gas mass at a startling rate of ≳10,000 M⊙ yr−1. A broad component that is red-shifted from the galaxy emission is detected in four (low and high J) CO and [C I] transitions and in the ionized phase, which ensures a robust estimate of the expelled gas mass. The implied statistics suggest that similar events are potentially a major star-formation quenching channel. However, our observations provide compelling evidence that this is not a feedback-driven wind, but rather material from a merger that has been probably tidally ejected. This finding challenges some literature studies in which the role of feedback-driven winds might be overstated.es
dc.description.sponsorshipA.P. and E.D. thank A. Renzini for commenting on the manuscript and for useful discussion. A.P. acknowledges funding from Region Île-de-France and an Incoming CEA fellowship from the CEA-Enhanced Eurotalents programme, co-funded by the FP7 Marie-Skłodowska-Curie COFUND programme (grant agreement 600382). A.P. also gratefully acknowledges financial support from the STFC (grants ST/T000244/1 and ST/P000541/1). M.P. acknowledges support from the Comunidad de Madrid through the Atracción de Talento Investigador (grant 2018-T1/TIC-11035). S.J. acknowledges financial support from the Spanish Ministry of Science, Innovation and Universities (MICIU) (grant AYA2017-84061-P), co-financed by FEDER (European Regional Development Funds).es
dc.language.isoenges
dc.publisherNature Research Journalses
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2017-84061-P/ES/DE LAS PRIMERAS SOBRE-DENSIDADES A LOS PROTO-CUMULOS Y CUMULOS: EL PAPEL DEL ENTORNO/-
dc.subjectGalaxies and clusterses
dc.subjectInterstellar mediumes
dc.titleA titanic interstellar medium ejection from a massive starburst galaxy at redshift 1.4es
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcidDelvecchio, I. [0000-0001-8706-2252]-
dc.contributor.orcidEnia, A. [0000-0002-0200-2857]-
dc.contributor.orcidDaddi, E. [0000-0002-3331-9590]-
dc.contributor.orcidValentino, F. [0000-0001-6477-4011]-
dc.contributor.orcidMancini, C. [0000-0002-4297-0561]-
dc.contributor.orcidLiu, D. [0000-0001-9773-7479]-
dc.identifier.doi10.1038/s41550-020-01268-x-
dc.identifier.e-issn2397-3366-
dc.contributor.funderScience and Technology Facilities Council (STFC)-
dc.contributor.funderEuropean Regional Development Fund (ERDF)-
dc.contributor.funderEuropean Commission (EC)-
dc.contributor.funderComunidad de Madrid-
dc.description.peerreviewedPeerreviewes
dc.relation.publisherversionhttps://www.nature.com/articles/s41550-020-01268-xes
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000271-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000780-
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/restrictedAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/FP7/600382-
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