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dc.contributor.authorPović, Mirjanaes_ES
dc.contributor.authorMárquez, Isabeles_ES
dc.contributor.authorNetzer, Hagaies_ES
dc.contributor.authorMasegosa, Josefaes_ES
dc.contributor.authorNordon, Raananes_ES
dc.contributor.authorPérez Jiménez, Enriquees_ES
dc.contributor.authorSchoenell, Williames_ES
dc.date.accessioned2016-11-15T11:35:56Z-
dc.date.available2016-11-15T11:35:56Z-
dc.date.issued2016-07-28-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society 462(3): 2878-2903 (2016)es_ES
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10261/140225-
dc.description.abstractThis work presents the properties of 42 objects in the group of the most luminous, highest star formation rate (SFR) low-ionization nuclear emission-line regions (LINERs) at z = 0.04-0.11. We obtained long-slit spectroscopy of the nuclear regions for all sources, and FIR data (Herschel and IRAS) for 13 of them. We measured emission-line intensities, extinction, stellar populations, stellarmasses, ages, active galactic nuclei (AGN) luminosities, and SFRs. We find considerable differences from other low-redshift LINERs, in terms of extinction, and general similarity to star-forming galaxies. We confirm the existence of such luminous LINERs in the local universe, after being previously detected at z ~0.3 by Tommasin et al. Themedian stellar mass of these LINERs corresponds to 6-7 × 1010 M⊙ which was found in previous work to correspond to the peak of relative growth rate of stellar populations and therefore for the highest SFRs. Other LINERs although showing similar AGN luminosities have lower SFR. We find that most of these sources have LAGN ~ LSF suggesting co-evolution of black hole and stellarmass. In general, the fraction of local LINERs on themain sequence of star-forming galaxies is related to their AGN luminosity. © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.es_ES
dc.description.sponsorshipThis research was supported by the Junta de Andalucia through project TIC114, and the Spanish Ministry of Economy and Competitiveness (MINECO) through project AYA2013-42227-P. The work was also supported by the Israel Science Foundation grant 284/13. MP acknowledge financial support from JAE-Doc programme of the Spanish National Research Council (CSIC), co-funded by the European Social Fund.es_ES
dc.language.isoenges_ES
dc.publisherOxford University Presses_ES
dc.relationMINECO/ICTI2013-2016/AYA2013-42227-Pes_ES
dc.relation.isversionofPublisher's versiones_ES
dc.rightsopenAccessen_EN
dc.subjectGalaxies: activees_ES
dc.subjectGalaxies: nucleies_ES
dc.subjectGalaxies: star formationes_ES
dc.titleStar formation and AGN activity in the most luminous LINERs in the local universees_ES
dc.typeartículoes_ES
dc.identifier.doi10.1093/mnras/stw1842-
dc.description.peerreviewedPeer reviewedes_ES
dc.relation.publisherversionhttp://dx.doi.org/10.1093/mnras/stw1842es_ES
dc.identifier.e-issn1365-2966-
dc.embargo.terms2017-07-28es_ES
dc.contributor.funderJunta de Andalucíaes_ES
dc.contributor.funderMinisterio de Economía y Competitividad (España)es_ES
dc.contributor.funderIsrael Science Foundationes_ES
dc.contributor.funderConsejo Superior de Investigaciones Científicas (España)es_ES
dc.relation.csices_ES
oprm.item.hasRevisionno ko 0 false*
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003329es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003977es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003339es_ES
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