Please use this identifier to cite or link to this item: http://repositorio.unicamp.br/jspui/handle/REPOSIP/102490
Type: Artigo de periódico
Title: Merging Of Low-mass Systems And The Origin Of The Fundamental Plane
Author: Evstigneeva E.A.
De Carvalho R.R.
Ribeiro A.L.
Capelato H.V.
Abstract: We present the preliminary results of a study of how small stellar systems merge to form larger ones. As we display the families of galaxies in the μe - Re plane (effective surface brightness versus effective radius) we realize that different morphological types occupy different loci, evidencing the different physical mechanisms operating in each family. As proposed by Capaccioli et al. (1992) this diagram is the logical equivalent of the HR diagram for stars. Here we take some initial steps in understanding of how we can establish the evolutionary tracks, solely due to dynamical processes, in the μe - Re plane, ultimately making a dwarf elliptical to turn into a normal elliptical galaxy.
Editor: 
Rights: fechado
Identifier DOI: 10.1023/A:1024052110179
Address: http://www.scopus.com/inward/record.url?eid=2-s2.0-0347758384&partnerID=40&md5=29c22c06a1647c1cdc525dad0839de45
Date Issue: 2003
Appears in Collections:Unicamp - Artigos e Outros Documentos

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