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dc.contributor.authorCourtois, H. M.
dc.contributor.authorDomínguez Gómez, Jesús
dc.contributor.authorFlorido Navio, Estrella 
dc.contributor.authorGarcía Benito, Rubén
dc.contributor.authorPérez Martín, María Isabel 
dc.date.accessioned2023-06-22T07:31:06Z
dc.date.available2023-06-22T07:31:06Z
dc.date.issued2023-03-28
dc.identifier.citationCourtois, H. M., et al.: A&A 673, A38 (2023) [https://doi.org/10.1051/0004-6361/202245578]es_ES
dc.identifier.urihttps://hdl.handle.net/10481/82706
dc.description.abstractThe present study addresses a key question related to our understanding of the relation between void galaxies and their environment: the relationship between luminous and dark matter in and around voids. Aims. To explore the extent to which local Universe voids are empty of matter, we study the full (dark+luminous) matter content of seven nearby cosmic voids that are fully contained within the CosmicFlows-3 volume. Methods. We obtained the matter-density profiles of seven cosmic voids using two independent methods. These were built from the galaxy redshift space two-point correlation function in conjunction with peculiar velocity gradients from the CosmicFlows-3 dataset. Results. The results are striking, because when the redshift survey is used, all voids show a radial positive gradient of galaxies, while based on the dynamical analysis, only three of these voids display a clear underdensity of matter in their center. Conclusions. This work constitutes the most detailed observational analysis of voids conducted so far, and shows that void emptiness should be derived from dynamical information. From this limited study, the Hercules void appears to be the best candidate for a local Universe pure “pristine volume”, expanding in three directions with no dark matter located in that void.es_ES
dc.description.sponsorshipInstitut Universitaire de Francees_ES
dc.description.sponsorshipCentre National D'etudes Spatialeses_ES
dc.description.sponsorshipInstituto de Salud Carlos III Spanish Governmentes_ES
dc.description.sponsorshipEuropean Commission PID2020-224414GB-I00 PID2020-113689GB-I00es_ES
dc.description.sponsorshipSpanish Ministerio de Ciencia e Innovacion (MCIN)es_ES
dc.description.sponsorshipAgencia Estatal de Investigacion (AEI)es_ES
dc.description.sponsorshipEuropean Social Fund (ESF) 20215AT016 CEX2020-001058-Mes_ES
dc.description.sponsorshipCentro Superior de Investigaciones Cientificas (CSIC) under the PIE project KR4598/2-1es_ES
dc.description.sponsorshipGerman Research Foundation (DFG) PID2019-105602GBI00es_ES
dc.description.sponsorshipJunta de Andaluciaes_ES
dc.description.sponsorshipSpanish Government FQM108es_ES
dc.description.sponsorshipMCIN/AEIes_ES
dc.description.sponsorshipEuropean Union NextGenerationEUes_ES
dc.description.sponsorshipAgencia Estatal de Investigacion Espanola (AEI)es_ES
dc.description.sponsorshipCenter for Forestry Research & Experimentation (CIEF) CEX2021-001131-Ses_ES
dc.description.sponsorshipEuropean Union-Next Generation EU Fundses_ES
dc.description.sponsorshipState Research Agency (AEI-MCINN) of the Spanish Ministry of Science and Innovation under the grant "The structure and evolution of galaxies and their central regions" - Ministry of Universitieses_ES
dc.language.isoenges_ES
dc.publisherEDP Scienceses_ES
dc.rightsAtribución 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.subjectLarge-scale structure of Universees_ES
dc.subjectDark Matteres_ES
dc.titleSociology and hierarchy of voids: A study of seven nearby CAVITY galaxy voids and their dynamical CosmicFlows-3 environmentes_ES
dc.typejournal articlees_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/NextGenerationEU/PRTR-C17.I1es_ES
dc.rights.accessRightsopen accesses_ES
dc.identifier.doi10.1051/0004-6361/202245578
dc.type.hasVersionVoRes_ES


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Atribución 4.0 Internacional
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