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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/144422
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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 Técnicas2025-09-29T10:17:15Zoai: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:34982025-09-29 10:17:15.995CONICET 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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1844614124541050880 |
score |
13.070432 |