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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/11236
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T10:20:45Zoai: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:34982025-09-29 10:20:45.498CONICET 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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1844614190885502976 |
score |
13.070432 |