dc.creatorDantas, CC
dc.creatorCapelato, HV
dc.creatorde Carvalho, RR
dc.creatorRibeiro, ALB
dc.date2002
dc.dateMAR
dc.date2014-11-20T04:08:13Z
dc.date2015-11-26T16:05:19Z
dc.date2014-11-20T04:08:13Z
dc.date2015-11-26T16:05:19Z
dc.date.accessioned2018-03-28T22:54:18Z
dc.date.available2018-03-28T22:54:18Z
dc.identifierAstronomy & Astrophysics. E D P Sciences, v. 384, n. 3, n. 772, n. 779, 2002.
dc.identifier0004-6361
dc.identifierWOS:000174448600006
dc.identifier10.1051/0004-6361:20020073
dc.identifierhttp://www.repositorio.unicamp.br/jspui/handle/REPOSIP/62533
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/62533
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/62533
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1265672
dc.descriptionFollowing on from the numerical work of Capelato et al. (1995, 1997), where dissipationless merger simulations were shown to reproduce the "Fundamental Plane" (FP) of elliptical galaxies, we investigate whether the end products of pure, spherically symmetric, one-component dissipationless collapses could also reproduce the FP. Past numerical work on collisionless collapses have addressed important issues on the dynamical/structural characteristics of collapsed equilibrium systems. However, the study of collisionless collapse in the context of the nature of the FP has not been satisfactorily addressed yet. Our aim in this paper is to focus our attention on the resulting collapse of simple one-component spherical models with a range of different initial virial coefficients. We find that the characteristic correlations of the models are compatible with virialized, centrally homologous systems. Our results strengthen the idea that merging may be a fundamental ingredient in forming non-homologous objects.
dc.description384
dc.description3
dc.description772
dc.description779
dc.languageen
dc.publisherE D P Sciences
dc.publisherLes Ulis Cedexa
dc.publisherFrança
dc.relationAstronomy & Astrophysics
dc.relationAstron. Astrophys.
dc.rightsaberto
dc.sourceWeb of Science
dc.subjectgalaxies : elliptical midlenticular, cD
dc.subjectgalaxies : fundamental parameters
dc.subjectmethods : numerical
dc.subjectElliptic Galaxies
dc.subjectStellar-systems
dc.subjectPhysical-properties
dc.subjectViolent Relaxation
dc.subjectVirial-theorem
dc.subjectStability
dc.subjectMergers
dc.subjectClues
dc.subjectField
dc.titleDissipationless collapse of spherical protogalaxies and the fundamental plane
dc.typeArtículos de revistas


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