About the linearity of the color-magnitude relation of early-type galaxies in the Virgo Cluster

We revisit the color-magnitude relation of Virgo Cluster early-type galaxies in order to explore its alleged nonlinearity. To this aim, we reanalyze the relation already published from data obtained within the ACS Virgo Cluster Survey of the Hubble Space Telescope and perform our own photometry and...

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Autores principales: Smith Castelli, Analía Viviana, González, Nélida Mabel, Faifer, Favio Raúl, Forte, Juan Carlos
Formato: Articulo
Lenguaje:Inglés
Publicado: 2013
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/85350
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id I19-R120-10915-85350
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
galaxies: clusters: general
galaxies: clusters: individual (Virgo)
galaxies: dwarf
galaxies: elliptical and lenticular, cD
galaxies: photometry
spellingShingle Ciencias Astronómicas
galaxies: clusters: general
galaxies: clusters: individual (Virgo)
galaxies: dwarf
galaxies: elliptical and lenticular, cD
galaxies: photometry
Smith Castelli, Analía Viviana
González, Nélida Mabel
Faifer, Favio Raúl
Forte, Juan Carlos
About the linearity of the color-magnitude relation of early-type galaxies in the Virgo Cluster
topic_facet Ciencias Astronómicas
galaxies: clusters: general
galaxies: clusters: individual (Virgo)
galaxies: dwarf
galaxies: elliptical and lenticular, cD
galaxies: photometry
description We revisit the color-magnitude relation of Virgo Cluster early-type galaxies in order to explore its alleged nonlinearity. To this aim, we reanalyze the relation already published from data obtained within the ACS Virgo Cluster Survey of the Hubble Space Telescope and perform our own photometry and analysis of the images of 100 early-type galaxies observed as part of this survey. In addition, we compare our results with those reported in the literature from data of the Sloan Digital Sky Survey. We have found that when the brightest galaxies and untypical systems are excluded from the sample, a linear relation arises in agreement with what is observed in other groups and clusters. The central regions of the brightest galaxies also follow this relation. In addition, we notice that Virgo contains at least four compact elliptical galaxies besides the well-known object VCC 1297 (NGC 4486B). Their locations in the 〈μeff〉-luminosity diagram define a trend different from that followed by normal early-type dwarf galaxies, setting an upper limit in effective surface brightness and a lower limit in the effective radius for their luminosities. Based on the distribution of different galaxy sub-samples in the color-magnitude and 〈μeff〉-luminosity diagrams, we draw some conclusions on their formation and the history of their evolution.
format Articulo
Articulo
author Smith Castelli, Analía Viviana
González, Nélida Mabel
Faifer, Favio Raúl
Forte, Juan Carlos
author_facet Smith Castelli, Analía Viviana
González, Nélida Mabel
Faifer, Favio Raúl
Forte, Juan Carlos
author_sort Smith Castelli, Analía Viviana
title About the linearity of the color-magnitude relation of early-type galaxies in the Virgo Cluster
title_short About the linearity of the color-magnitude relation of early-type galaxies in the Virgo Cluster
title_full About the linearity of the color-magnitude relation of early-type galaxies in the Virgo Cluster
title_fullStr About the linearity of the color-magnitude relation of early-type galaxies in the Virgo Cluster
title_full_unstemmed About the linearity of the color-magnitude relation of early-type galaxies in the Virgo Cluster
title_sort about the linearity of the color-magnitude relation of early-type galaxies in the virgo cluster
publishDate 2013
url http://sedici.unlp.edu.ar/handle/10915/85350
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