dc.creatorPérez, Josefa
dc.creatorTissera, Patricia Beatriz
dc.creatorLambas, Diego G.
dc.creatorScannapieco, Cecilia
dc.date2005-12
dc.date2007
dc.date2021-08-30T18:53:29Z
dc.date.accessioned2023-07-15T02:50:21Z
dc.date.available2023-07-15T02:50:21Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/123775
dc.identifierisbn:978-3-642-09026-4
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7463466
dc.descriptionWe carry out a statistical analysis of galaxy pairs selected from chemical hydrodynamical simulations with the aim at assessing the capability of hierarchical scenarios to reproduce recent observational results for galaxies in pairs. Particularly, we analyse the effects of mergers and interactions on the star formation (SF) activity, the global mean chemical properties and the colour distribution of interacting galaxies. We also assess the effects of spurious pairs.
dc.descriptionPublicado en <i>Groups of Galaxies in the Nearby Universe. ESO Astrophysics Symposia book series</i>
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format239-240
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsCreative Commons Attribution 4.0 International (CC BY 4.0)
dc.subjectCiencias Astronómicas
dc.subjectStar Forma
dc.subjectColour Distribution
dc.subjectTidal Interaction
dc.subjectChemical Abundance
dc.titleThe role of tidal interactions in driving galaxy evolution
dc.typeObjeto de conferencia
dc.typeObjeto de conferencia


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