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

Autores
Smith Castelli, Analia Viviana; Gonzalez, Nelida Mabel; Faifer, Favio Raúl; Forte, Juan Carlos
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
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.
Fil: Smith Castelli, Analia Viviana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata; Argentina
Fil: Gonzalez, Nelida Mabel. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Universidad Nacional de la Plata; Argentina
Fil: Faifer, Favio Raúl. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Forte, Juan Carlos. Gobierno de la Ciudad de Buenos Aires. Secretaria de Cultura. Subsecretaria de Patrimonio Cultural. Planetario "galileo Galilei"; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Materia
Galaxeis
Clusters
Virgo
Dwarf
Elliptical galaxies
Lenticular galaxies
Photometry
Nivel de accesibilidad
acceso abierto
Condiciones de uso
Atribución-NoComercial-CompartirIgual 2.5 Argentina (CC BY-NC-SA 2.5 AR)
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/11236
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/11236
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling About the linearity of the color-magnitude relation of early-type galaxies in the Virgo clusterSmith Castelli, Analia VivianaGonzalez, Nelida MabelFaifer, Favio RaúlForte, Juan CarlosGalaxeisClustersVirgoDwarfElliptical galaxiesLenticular galaxiesPhotometryhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We 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.Fil: Smith Castelli, Analia Viviana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata; ArgentinaFil: Gonzalez, Nelida Mabel. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Universidad Nacional de la Plata; ArgentinaFil: Faifer, Favio Raúl. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Forte, Juan Carlos. Gobierno de la Ciudad de Buenos Aires. Secretaria de Cultura. Subsecretaria de Patrimonio Cultural. Planetario "galileo Galilei"; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaIop Publishing2013-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/11236Smith Castelli, Analia Viviana; Gonzalez, Nelida Mabel; Faifer, Favio Raúl; Forte, Juan Carlos; About the linearity of the color-magnitude relation of early-type galaxies in the Virgo cluster; Iop Publishing; Astrophysical Journal; 772; 1; 6-2013; 68-790004-637Xenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/772/1/68/metainfo:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/772/1/68info:eu-repo/semantics/openAccessAtribución-NoComercial-CompartirIgual 2.5 Argentina (CC BY-NC-SA 2.5 AR)https://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:53:26Zoai:ri.conicet.gov.ar:11336/11236instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:53:26.421CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv About the linearity of the color-magnitude relation of early-type galaxies in the Virgo cluster
title About the linearity of the color-magnitude relation of early-type galaxies in the Virgo cluster
spellingShingle About the linearity of the color-magnitude relation of early-type galaxies in the Virgo cluster
Smith Castelli, Analia Viviana
Galaxeis
Clusters
Virgo
Dwarf
Elliptical galaxies
Lenticular galaxies
Photometry
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
dc.creator.none.fl_str_mv Smith Castelli, Analia Viviana
Gonzalez, Nelida Mabel
Faifer, Favio Raúl
Forte, Juan Carlos
author Smith Castelli, Analia Viviana
author_facet Smith Castelli, Analia Viviana
Gonzalez, Nelida Mabel
Faifer, Favio Raúl
Forte, Juan Carlos
author_role author
author2 Gonzalez, Nelida Mabel
Faifer, Favio Raúl
Forte, Juan Carlos
author2_role author
author
author
dc.subject.none.fl_str_mv Galaxeis
Clusters
Virgo
Dwarf
Elliptical galaxies
Lenticular galaxies
Photometry
topic Galaxeis
Clusters
Virgo
Dwarf
Elliptical galaxies
Lenticular galaxies
Photometry
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv 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.
Fil: Smith Castelli, Analia Viviana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina. Universidad Nacional de la Plata; Argentina
Fil: Gonzalez, Nelida Mabel. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Universidad Nacional de la Plata; Argentina
Fil: Faifer, Favio Raúl. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Forte, Juan Carlos. Gobierno de la Ciudad de Buenos Aires. Secretaria de Cultura. Subsecretaria de Patrimonio Cultural. Planetario "galileo Galilei"; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
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.
publishDate 2013
dc.date.none.fl_str_mv 2013-06
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/11236
Smith Castelli, Analia Viviana; Gonzalez, Nelida Mabel; Faifer, Favio Raúl; Forte, Juan Carlos; About the linearity of the color-magnitude relation of early-type galaxies in the Virgo cluster; Iop Publishing; Astrophysical Journal; 772; 1; 6-2013; 68-79
0004-637X
url http://hdl.handle.net/11336/11236
identifier_str_mv Smith Castelli, Analia Viviana; Gonzalez, Nelida Mabel; Faifer, Favio Raúl; Forte, Juan Carlos; About the linearity of the color-magnitude relation of early-type galaxies in the Virgo cluster; Iop Publishing; Astrophysical Journal; 772; 1; 6-2013; 68-79
0004-637X
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/772/1/68/meta
info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/772/1/68
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
Atribución-NoComercial-CompartirIgual 2.5 Argentina (CC BY-NC-SA 2.5 AR)
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv Atribución-NoComercial-CompartirIgual 2.5 Argentina (CC BY-NC-SA 2.5 AR)
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv Iop Publishing
publisher.none.fl_str_mv Iop Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 12.982451

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