Early-type galaxies in the Antlia Cluster: global properties

Autores
Calderón, Juan Pablo; Bassino, Lilia Patricia; Cellone, Sergio Aldo; Gómez, Matias; Caso, Juan Pablo
Año de publicación
2020
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We presentan extension of our previous research on the early-type galaxy population ofthe Antlia cluster (d ~ 35 Mpc), achieving a total coverage of ~ 2.6 deg x degand performing surface photometry for ~300 galaxies, 130 of which are newuncatalogued ones. Such new galaxies mainly fall in the low surface brightness(LSB) regime, but there are also some lenticulars (S0) which support theexistence of unique functions that connect bright and dwarf galaxies in thescaling relations. We analyse the projected spatial distribution of galaxies upto a distance of ~800 kpc from NGC 3268, the adopted centre, as well as theradial velocity distribution and the correlation between galaxy colour andeffective radius with the projected spatial distribution. We also obtain theluminosity function of the early-type galaxies and the distribution of stellarmasses using the T1-band magnitudes and adopted mass-luminosity ratios.Additionally, we correlate the central galaxy distribution with an X-rayemission map from the literature. Based on the analysis of the radialvelocities and galaxy colour distributions, we find that galaxies redder thanthe colour-magnitude relation (CMR) have a velocity distribution stronglyconcentrated towards the values of the dominant galaxies and are homogeneouslydistributed throughout the cluster. Those bluer than the CMR, in turn, have amuch more extended radial velocity distribution and are concentrated towardsthe centre of the cluster. We also identify 12 candidates to ultra diffuse galaxies(UDG), that seem to be split into two families, and speculate about theirorigins in the context of the cluster structure.
Fil: Calderón, Juan Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Bassino, Lilia Patricia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Gómez, Matias. Departamento de Astronomia; Chile
Fil: Caso, Juan Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Materia
GALAXY CLUSTER
DWARF GALAXIES
STRUCTURAL PARAMETERS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/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:11336/144422
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/144422
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Early-type galaxies in the Antlia Cluster: global propertiesCalderón, Juan PabloBassino, Lilia PatriciaCellone, Sergio AldoGómez, MatiasCaso, Juan PabloGALAXY CLUSTERDWARF GALAXIESSTRUCTURAL PARAMETERShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We presentan extension of our previous research on the early-type galaxy population ofthe Antlia cluster (d ~ 35 Mpc), achieving a total coverage of ~ 2.6 deg x degand performing surface photometry for ~300 galaxies, 130 of which are newuncatalogued ones. Such new galaxies mainly fall in the low surface brightness(LSB) regime, but there are also some lenticulars (S0) which support theexistence of unique functions that connect bright and dwarf galaxies in thescaling relations. We analyse the projected spatial distribution of galaxies upto a distance of ~800 kpc from NGC 3268, the adopted centre, as well as theradial velocity distribution and the correlation between galaxy colour andeffective radius with the projected spatial distribution. We also obtain theluminosity function of the early-type galaxies and the distribution of stellarmasses using the T1-band magnitudes and adopted mass-luminosity ratios.Additionally, we correlate the central galaxy distribution with an X-rayemission map from the literature. Based on the analysis of the radialvelocities and galaxy colour distributions, we find that galaxies redder thanthe colour-magnitude relation (CMR) have a velocity distribution stronglyconcentrated towards the values of the dominant galaxies and are homogeneouslydistributed throughout the cluster. Those bluer than the CMR, in turn, have amuch more extended radial velocity distribution and are concentrated towardsthe centre of the cluster. We also identify 12 candidates to ultra diffuse galaxies(UDG), that seem to be split into two families, and speculate about theirorigins in the context of the cluster structure.Fil: Calderón, Juan Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Bassino, Lilia Patricia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Gómez, Matias. Departamento de Astronomia; ChileFil: Caso, Juan Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaWiley Blackwell Publishing, Inc2020-07info: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/11336/144422Calderón, Juan Pablo; Bassino, Lilia Patricia; Cellone, Sergio Aldo; Gómez, Matias ; Caso, Juan Pablo; Early-type galaxies in the Antlia Cluster: global properties; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 497; 7-2020; 1791-18060035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/497/2/1791/5870689info:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1093/mnras/staa2043info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:47:24Zoai:ri.conicet.gov.ar:11336/144422instacron: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 11:47:24.702CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Early-type galaxies in the Antlia Cluster: global properties
title Early-type galaxies in the Antlia Cluster: global properties
spellingShingle Early-type galaxies in the Antlia Cluster: global properties
Calderón, Juan Pablo
GALAXY CLUSTER
DWARF GALAXIES
STRUCTURAL PARAMETERS
title_short Early-type galaxies in the Antlia Cluster: global properties
title_full Early-type galaxies in the Antlia Cluster: global properties
title_fullStr Early-type galaxies in the Antlia Cluster: global properties
title_full_unstemmed Early-type galaxies in the Antlia Cluster: global properties
title_sort Early-type galaxies in the Antlia Cluster: global properties
dc.creator.none.fl_str_mv Calderón, Juan Pablo
Bassino, Lilia Patricia
Cellone, Sergio Aldo
Gómez, Matias
Caso, Juan Pablo
author Calderón, Juan Pablo
author_facet Calderón, Juan Pablo
Bassino, Lilia Patricia
Cellone, Sergio Aldo
Gómez, Matias
Caso, Juan Pablo
author_role author
author2 Bassino, Lilia Patricia
Cellone, Sergio Aldo
Gómez, Matias
Caso, Juan Pablo
author2_role author
author
author
author
dc.subject.none.fl_str_mv GALAXY CLUSTER
DWARF GALAXIES
STRUCTURAL PARAMETERS
topic GALAXY CLUSTER
DWARF GALAXIES
STRUCTURAL PARAMETERS
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 presentan extension of our previous research on the early-type galaxy population ofthe Antlia cluster (d ~ 35 Mpc), achieving a total coverage of ~ 2.6 deg x degand performing surface photometry for ~300 galaxies, 130 of which are newuncatalogued ones. Such new galaxies mainly fall in the low surface brightness(LSB) regime, but there are also some lenticulars (S0) which support theexistence of unique functions that connect bright and dwarf galaxies in thescaling relations. We analyse the projected spatial distribution of galaxies upto a distance of ~800 kpc from NGC 3268, the adopted centre, as well as theradial velocity distribution and the correlation between galaxy colour andeffective radius with the projected spatial distribution. We also obtain theluminosity function of the early-type galaxies and the distribution of stellarmasses using the T1-band magnitudes and adopted mass-luminosity ratios.Additionally, we correlate the central galaxy distribution with an X-rayemission map from the literature. Based on the analysis of the radialvelocities and galaxy colour distributions, we find that galaxies redder thanthe colour-magnitude relation (CMR) have a velocity distribution stronglyconcentrated towards the values of the dominant galaxies and are homogeneouslydistributed throughout the cluster. Those bluer than the CMR, in turn, have amuch more extended radial velocity distribution and are concentrated towardsthe centre of the cluster. We also identify 12 candidates to ultra diffuse galaxies(UDG), that seem to be split into two families, and speculate about theirorigins in the context of the cluster structure.
Fil: Calderón, Juan Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Bassino, Lilia Patricia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Gómez, Matias. Departamento de Astronomia; Chile
Fil: Caso, Juan Pablo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
description We presentan extension of our previous research on the early-type galaxy population ofthe Antlia cluster (d ~ 35 Mpc), achieving a total coverage of ~ 2.6 deg x degand performing surface photometry for ~300 galaxies, 130 of which are newuncatalogued ones. Such new galaxies mainly fall in the low surface brightness(LSB) regime, but there are also some lenticulars (S0) which support theexistence of unique functions that connect bright and dwarf galaxies in thescaling relations. We analyse the projected spatial distribution of galaxies upto a distance of ~800 kpc from NGC 3268, the adopted centre, as well as theradial velocity distribution and the correlation between galaxy colour andeffective radius with the projected spatial distribution. We also obtain theluminosity function of the early-type galaxies and the distribution of stellarmasses using the T1-band magnitudes and adopted mass-luminosity ratios.Additionally, we correlate the central galaxy distribution with an X-rayemission map from the literature. Based on the analysis of the radialvelocities and galaxy colour distributions, we find that galaxies redder thanthe colour-magnitude relation (CMR) have a velocity distribution stronglyconcentrated towards the values of the dominant galaxies and are homogeneouslydistributed throughout the cluster. Those bluer than the CMR, in turn, have amuch more extended radial velocity distribution and are concentrated towardsthe centre of the cluster. We also identify 12 candidates to ultra diffuse galaxies(UDG), that seem to be split into two families, and speculate about theirorigins in the context of the cluster structure.
publishDate 2020
dc.date.none.fl_str_mv 2020-07
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/11336/144422
Calderón, Juan Pablo; Bassino, Lilia Patricia; Cellone, Sergio Aldo; Gómez, Matias ; Caso, Juan Pablo; Early-type galaxies in the Antlia Cluster: global properties; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 497; 7-2020; 1791-1806
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/144422
identifier_str_mv Calderón, Juan Pablo; Bassino, Lilia Patricia; Cellone, Sergio Aldo; Gómez, Matias ; Caso, Juan Pablo; Early-type galaxies in the Antlia Cluster: global properties; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 497; 7-2020; 1791-1806
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/497/2/1791/5870689
info:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1093/mnras/staa2043
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv 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 Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
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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