The Abell 85 BCG: A Nucleated, Coreless Galaxy
- Autores
- Madrid, Juan P.; Donzelli, Carlos Jose
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- New high-resolution r-band imaging of the brightest cluster galaxy (BCG) in Abell 85 (Holm 15A) was obtained using the Gemini Multi Object Spectrograph. These data were taken with the aim of deriving an accurate surface brightness profile of the BCG of Abell 85, in particular, its central region. The new Gemini data show clear evidence of a previously unreported nuclear emission that is evident as a distinct light excess in the central kiloparsec of the surface brightness profile. We find that the light profile is never flat nor does it present a downward trend toward the center of the galaxy. That is, the new Gemini data show a different physical reality from the featureless, "evacuated core" recently claimed for the Abell 85 BCG. After trying different models, we find that the surface brightness profile of the BCG of Abell 85 is best fit by a double Sérsic model.
Fil: Madrid, Juan P.. Gemini Observatorysouthern Operations Center; Chile. Commonwealth Scientific And Industrial Research Organization; Australia
Fil: Donzelli, Carlos Jose. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina - Materia
-
GALAXIES: CLUSTERS: GENERAL
GALAXIES: INDIVIDUAL (ABELL 85, HOLM 15A)
GALAXIES: NUCLEI
GALAXIES: STRUCTURE - 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:11336/183615
Ver los metadatos del registro completo
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spelling |
The Abell 85 BCG: A Nucleated, Coreless GalaxyMadrid, Juan P.Donzelli, Carlos JoseGALAXIES: CLUSTERS: GENERALGALAXIES: INDIVIDUAL (ABELL 85, HOLM 15A)GALAXIES: NUCLEIGALAXIES: STRUCTUREhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1New high-resolution r-band imaging of the brightest cluster galaxy (BCG) in Abell 85 (Holm 15A) was obtained using the Gemini Multi Object Spectrograph. These data were taken with the aim of deriving an accurate surface brightness profile of the BCG of Abell 85, in particular, its central region. The new Gemini data show clear evidence of a previously unreported nuclear emission that is evident as a distinct light excess in the central kiloparsec of the surface brightness profile. We find that the light profile is never flat nor does it present a downward trend toward the center of the galaxy. That is, the new Gemini data show a different physical reality from the featureless, "evacuated core" recently claimed for the Abell 85 BCG. After trying different models, we find that the surface brightness profile of the BCG of Abell 85 is best fit by a double Sérsic model.Fil: Madrid, Juan P.. Gemini Observatorysouthern Operations Center; Chile. Commonwealth Scientific And Industrial Research Organization; AustraliaFil: Donzelli, Carlos Jose. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaIOP Publishing2016-02-26info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/183615Madrid, Juan P.; Donzelli, Carlos Jose; The Abell 85 BCG: A Nucleated, Coreless Galaxy; IOP Publishing; Astrophysical Journal; 819; 1; 26-2-2016; 50-570004-637X1538-4357CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/0004-637X/819/1/50info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/0004-637X/819/1/50info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:33:41Zoai:ri.conicet.gov.ar:11336/183615instacron: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 09:33:42.061CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The Abell 85 BCG: A Nucleated, Coreless Galaxy |
title |
The Abell 85 BCG: A Nucleated, Coreless Galaxy |
spellingShingle |
The Abell 85 BCG: A Nucleated, Coreless Galaxy Madrid, Juan P. GALAXIES: CLUSTERS: GENERAL GALAXIES: INDIVIDUAL (ABELL 85, HOLM 15A) GALAXIES: NUCLEI GALAXIES: STRUCTURE |
title_short |
The Abell 85 BCG: A Nucleated, Coreless Galaxy |
title_full |
The Abell 85 BCG: A Nucleated, Coreless Galaxy |
title_fullStr |
The Abell 85 BCG: A Nucleated, Coreless Galaxy |
title_full_unstemmed |
The Abell 85 BCG: A Nucleated, Coreless Galaxy |
title_sort |
The Abell 85 BCG: A Nucleated, Coreless Galaxy |
dc.creator.none.fl_str_mv |
Madrid, Juan P. Donzelli, Carlos Jose |
author |
Madrid, Juan P. |
author_facet |
Madrid, Juan P. Donzelli, Carlos Jose |
author_role |
author |
author2 |
Donzelli, Carlos Jose |
author2_role |
author |
dc.subject.none.fl_str_mv |
GALAXIES: CLUSTERS: GENERAL GALAXIES: INDIVIDUAL (ABELL 85, HOLM 15A) GALAXIES: NUCLEI GALAXIES: STRUCTURE |
topic |
GALAXIES: CLUSTERS: GENERAL GALAXIES: INDIVIDUAL (ABELL 85, HOLM 15A) GALAXIES: NUCLEI GALAXIES: STRUCTURE |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
New high-resolution r-band imaging of the brightest cluster galaxy (BCG) in Abell 85 (Holm 15A) was obtained using the Gemini Multi Object Spectrograph. These data were taken with the aim of deriving an accurate surface brightness profile of the BCG of Abell 85, in particular, its central region. The new Gemini data show clear evidence of a previously unreported nuclear emission that is evident as a distinct light excess in the central kiloparsec of the surface brightness profile. We find that the light profile is never flat nor does it present a downward trend toward the center of the galaxy. That is, the new Gemini data show a different physical reality from the featureless, "evacuated core" recently claimed for the Abell 85 BCG. After trying different models, we find that the surface brightness profile of the BCG of Abell 85 is best fit by a double Sérsic model. Fil: Madrid, Juan P.. Gemini Observatorysouthern Operations Center; Chile. Commonwealth Scientific And Industrial Research Organization; Australia Fil: Donzelli, Carlos Jose. Observatorio Astronomico de la Universidad Nacional de Cordoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina |
description |
New high-resolution r-band imaging of the brightest cluster galaxy (BCG) in Abell 85 (Holm 15A) was obtained using the Gemini Multi Object Spectrograph. These data were taken with the aim of deriving an accurate surface brightness profile of the BCG of Abell 85, in particular, its central region. The new Gemini data show clear evidence of a previously unreported nuclear emission that is evident as a distinct light excess in the central kiloparsec of the surface brightness profile. We find that the light profile is never flat nor does it present a downward trend toward the center of the galaxy. That is, the new Gemini data show a different physical reality from the featureless, "evacuated core" recently claimed for the Abell 85 BCG. After trying different models, we find that the surface brightness profile of the BCG of Abell 85 is best fit by a double Sérsic model. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-02-26 |
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/11336/183615 Madrid, Juan P.; Donzelli, Carlos Jose; The Abell 85 BCG: A Nucleated, Coreless Galaxy; IOP Publishing; Astrophysical Journal; 819; 1; 26-2-2016; 50-57 0004-637X 1538-4357 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/183615 |
identifier_str_mv |
Madrid, Juan P.; Donzelli, Carlos Jose; The Abell 85 BCG: A Nucleated, Coreless Galaxy; IOP Publishing; Astrophysical Journal; 819; 1; 26-2-2016; 50-57 0004-637X 1538-4357 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.3847/0004-637X/819/1/50 info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/0004-637X/819/1/50 |
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 |
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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1844613036893011968 |
score |
13.070432 |