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dc.contributor.authorLyman, J. D.
dc.contributor.authorGalbany González, Lluis 
dc.contributor.authorSánchez, S. F.
dc.contributor.authorAnderson, J. P.
dc.contributor.authorKuncarayakti, H.
dc.date.accessioned2020-12-02T10:06:53Z
dc.date.available2020-12-02T10:06:53Z
dc.date.issued2020-05-01
dc.identifier.citationPublished version: Lyman, J. D., Galbany, L., Sánchez, S. F., Anderson, J. P., Kuncarayakti, H., & Prieto, J. L. (2020). Studying the environment of AT 2018cow with MUSE. Monthly Notices of the Royal Astronomical Society, 495(1), 992-999. [DOI:10.1093/mnras/staa1243]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/64587
dc.description.abstractAT2018cow was the nearest and best studied example of a new breed of extra-galactic, luminous and rapidly-evolving transient. Both the progenitor systems and explosion mechanisms of these rapid transients remain a mystery { the energetics, spectral signa- tures, and timescales make them challenging to interpret in established classes of super- novae and tidal disruption events. The rich, multi-wavelength data-set of AT2018cow has still left several interpretations viable to explain the nature of this event. In this paper we analyse integral- eld spectroscopic data of the host galaxy, CGCG137-068, to compare environmental constraints with leading progenitor models. We nd the explosion site of AT2018cow to be very typical of core-collapse supernovae (known to form from stars with MZAMS 8-25 M ), and infer a young stellar population age at the explosion site of few 10Myr, at slightly sub-solar metallicity. When comparing to expectations for exotic intermediate-mass black hole (IMBH) tidal disruption events, we nd no evidence for a potential host system of the IMBH. In particular, there are no abrupt changes in metallicity or kinematics in the vicinity of the explosion site, ar- guing against the presence of a distinct host system. The proximity of AT2018cow to strong star-formation in the host galaxy makes us favour a massive stellar progenitor for this event.es_ES
dc.description.sponsorshipScience & Technology Facilities Council (STFC) Science and Technology Development Fund (STDF) ST/P000495/1es_ES
dc.description.sponsorshipEuropean Union (EU) 839090es_ES
dc.description.sponsorshipEuropean Union (EU) PGC2018-095317-B-C21es_ES
dc.description.sponsorshipConsejo Nacional de Ciencia y Tecnologia (CONACyT) CB-285080 FC-2016-01-1916es_ES
dc.description.sponsorship(UNAM) project PAPIIT-DGAPA-IN100519es_ES
dc.description.sponsorshipEuropean Organisation for Astronomical Research in the Southern Hemisphere under ESO programme 0103.D-0440(A)es_ES
dc.language.isoenges_ES
dc.publisherOxford Univ Presses_ES
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.subjectStars: massivees_ES
dc.subjectSupernovae: generales_ES
dc.subjectSupernovae: individual: AT2018cowes_ES
dc.subjectGalaxies: individual: CGCG137-068es_ES
dc.titleStudying the environment of AT2018cow with MUSEes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/HORIZON2020/839090es_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.doi10.1093/mnras/staa1243
dc.type.hasVersioninfo:eu-repo/semantics/submittedVersiones_ES


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