Globular cluster systems as tracers of the evolutionary history in NGC 3258 and NGC 3268
- Autores
- Caso, Juan Pablo; Bassino, Lilia Patricia; Gómez, Matías
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present a new photometric study of NGC 3258 and NGC 3268 globular cluster systems (GCSs), using images in filters B, C, V, R, I and z', obtained from four different telescopes. The wide spatial coverage allows us to estimate the whole extension of both GCSs more precisely than in previous works, and new values for the richness of GC subpopulations. We find differences in the azimuthal distribution between blue (metal-poor) and red (metal-rich) globular clusters (GCs), and confirm that radial profiles flatten towards the centre of the galaxies. In both cases we detected a radial gradient in the colour peak of blue GCs which might be related to the construction of the GCSs. We analyse the similarities and differences in both GCSs, in the context of the possible evolutionary histories of the host galaxies. We also obtain photometric metallicities for a large number of GC candidates around NGC 3258, by applying multicolour-metallicity relations. These results confirm the bimodal metallicity distribution.
Instituto de Astrofísica de La Plata - Materia
-
Ciencias Astronómicas
Galaxies: elliptical and lenticular
Galaxies: evolution
Galaxies: star clusters: individual: NGC 3258 & NGC 3268 - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/93479
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Globular cluster systems as tracers of the evolutionary history in NGC 3258 and NGC 3268Caso, Juan PabloBassino, Lilia PatriciaGómez, MatíasCiencias AstronómicasGalaxies: elliptical and lenticularGalaxies: evolutionGalaxies: star clusters: individual: NGC 3258 & NGC 3268We present a new photometric study of NGC 3258 and NGC 3268 globular cluster systems (GCSs), using images in filters B, C, V, R, I and z', obtained from four different telescopes. The wide spatial coverage allows us to estimate the whole extension of both GCSs more precisely than in previous works, and new values for the richness of GC subpopulations. We find differences in the azimuthal distribution between blue (metal-poor) and red (metal-rich) globular clusters (GCs), and confirm that radial profiles flatten towards the centre of the galaxies. In both cases we detected a radial gradient in the colour peak of blue GCs which might be related to the construction of the GCSs. We analyse the similarities and differences in both GCSs, in the context of the possible evolutionary histories of the host galaxies. We also obtain photometric metallicities for a large number of GC candidates around NGC 3258, by applying multicolour-metallicity relations. These results confirm the bimodal metallicity distribution.Instituto de Astrofísica de La Plata2017-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf3227-3238http://sedici.unlp.edu.ar/handle/10915/93479enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx1393info:eu-repo/semantics/altIdentifier/hdl/11336/64625info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:19:26Zoai:sedici.unlp.edu.ar:10915/93479Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:19:26.926SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Globular cluster systems as tracers of the evolutionary history in NGC 3258 and NGC 3268 |
title |
Globular cluster systems as tracers of the evolutionary history in NGC 3258 and NGC 3268 |
spellingShingle |
Globular cluster systems as tracers of the evolutionary history in NGC 3258 and NGC 3268 Caso, Juan Pablo Ciencias Astronómicas Galaxies: elliptical and lenticular Galaxies: evolution Galaxies: star clusters: individual: NGC 3258 & NGC 3268 |
title_short |
Globular cluster systems as tracers of the evolutionary history in NGC 3258 and NGC 3268 |
title_full |
Globular cluster systems as tracers of the evolutionary history in NGC 3258 and NGC 3268 |
title_fullStr |
Globular cluster systems as tracers of the evolutionary history in NGC 3258 and NGC 3268 |
title_full_unstemmed |
Globular cluster systems as tracers of the evolutionary history in NGC 3258 and NGC 3268 |
title_sort |
Globular cluster systems as tracers of the evolutionary history in NGC 3258 and NGC 3268 |
dc.creator.none.fl_str_mv |
Caso, Juan Pablo Bassino, Lilia Patricia Gómez, Matías |
author |
Caso, Juan Pablo |
author_facet |
Caso, Juan Pablo Bassino, Lilia Patricia Gómez, Matías |
author_role |
author |
author2 |
Bassino, Lilia Patricia Gómez, Matías |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Galaxies: elliptical and lenticular Galaxies: evolution Galaxies: star clusters: individual: NGC 3258 & NGC 3268 |
topic |
Ciencias Astronómicas Galaxies: elliptical and lenticular Galaxies: evolution Galaxies: star clusters: individual: NGC 3258 & NGC 3268 |
dc.description.none.fl_txt_mv |
We present a new photometric study of NGC 3258 and NGC 3268 globular cluster systems (GCSs), using images in filters B, C, V, R, I and z', obtained from four different telescopes. The wide spatial coverage allows us to estimate the whole extension of both GCSs more precisely than in previous works, and new values for the richness of GC subpopulations. We find differences in the azimuthal distribution between blue (metal-poor) and red (metal-rich) globular clusters (GCs), and confirm that radial profiles flatten towards the centre of the galaxies. In both cases we detected a radial gradient in the colour peak of blue GCs which might be related to the construction of the GCSs. We analyse the similarities and differences in both GCSs, in the context of the possible evolutionary histories of the host galaxies. We also obtain photometric metallicities for a large number of GC candidates around NGC 3258, by applying multicolour-metallicity relations. These results confirm the bimodal metallicity distribution. Instituto de Astrofísica de La Plata |
description |
We present a new photometric study of NGC 3258 and NGC 3268 globular cluster systems (GCSs), using images in filters B, C, V, R, I and z', obtained from four different telescopes. The wide spatial coverage allows us to estimate the whole extension of both GCSs more precisely than in previous works, and new values for the richness of GC subpopulations. We find differences in the azimuthal distribution between blue (metal-poor) and red (metal-rich) globular clusters (GCs), and confirm that radial profiles flatten towards the centre of the galaxies. In both cases we detected a radial gradient in the colour peak of blue GCs which might be related to the construction of the GCSs. We analyse the similarities and differences in both GCSs, in the context of the possible evolutionary histories of the host galaxies. We also obtain photometric metallicities for a large number of GC candidates around NGC 3258, by applying multicolour-metallicity relations. These results confirm the bimodal metallicity distribution. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-09 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/93479 |
url |
http://sedici.unlp.edu.ar/handle/10915/93479 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0035-8711 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx1393 info:eu-repo/semantics/altIdentifier/hdl/11336/64625 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf 3227-3238 |
dc.source.none.fl_str_mv |
reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
reponame_str |
SEDICI (UNLP) |
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SEDICI (UNLP) |
instname_str |
Universidad Nacional de La Plata |
instacron_str |
UNLP |
institution |
UNLP |
repository.name.fl_str_mv |
SEDICI (UNLP) - Universidad Nacional de La Plata |
repository.mail.fl_str_mv |
alira@sedici.unlp.edu.ar |
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