The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster
- Autores
- Escudero, Carlos Gabriel; Cortesi, Arianna; Faifer, Favio Raúl; Sesto, Leandro Alberto; Smith Castelli, Analia Viviana; Johnston, Evelyn J.; Reynaldi, María Victoria; Chies Santos, Ana; Salinas, R.; Menendez Delmetre, Karín; S. Gonçalves, Thiago; Grossi, Marcos; Mendes de Oliveira, Claudia Lucia
- Año de publicación
- 2022
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- NGC 4382 is a merger-remnant galaxy that has been classified as morphological type E2, S0, and even Sa. In this work, we performed a photometric and spectroscopic analysis of the globular cluster (GC) system of this peculiar galaxy in order to provide additional information about its history. We used a combination of photometric data in different filters, and multiobject and long-slit spectroscopic data obtained using the Gemini/GMOS instrument. The photometric analysis of the GC system, using the Gaussian Mixture Model algorithm in the colour plane, reveals a complex colour distribution within Rgal < 5 arcmin (26.1 kpc), showing four different groups: the typical blue and red subpopulations, a group with intermediate colours, and the fourth group towards even redder colours. From the spectroscopic analysis of 47 GCs, confirmed members of NGC 4382 based on radial velocities, we verified 3 of the 4 photometric groups from the analysis of their stellar populations using the ULySS code. NGC 4382 presents the classic blue (10.4 ± 2.8 Gyr, [Fe/H] = -1.48 ± 0.18 dex), and red (12.1 ± 2.3 Gyr, [Fe/H] = -0.64 ± 0.26 dex) GCs formed earlier in the lifetime of the galaxy, and a third group of young GCs (2.2 ± 0.9 Gyr; [Fe/H] = -0.05 ± 0.28 dex). Finally, analysis of long-slit data of the galaxy reveals a luminosity-weighted mean age for the stellar population of ∼2.7 Gyr, and an increasing metallicity from [Fe/H] = -0.1 to +0.2 dex in Rgal < 10 arcsec (0.87 kpc). These values, and other morphological signatures in the galaxy, are in good agreement with the younger group of GCs, indicating a common origin as a result of a recent merger.
Fil: Escudero, Carlos Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. 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: Cortesi, Arianna. Universidade Federal do Rio de Janeiro; Brasil
Fil: Faifer, Favio Raúl. 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: Sesto, Leandro Alberto. Observatório Do Valongo; Brasil. 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: Smith Castelli, Analia Viviana. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. 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: Johnston, Evelyn J.. Universidad Diego Portales; Chile
Fil: Reynaldi, María Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. 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: Chies Santos, Ana. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Salinas, R.. Gemini Observatory; Chile
Fil: Menendez Delmetre, Karín. Universidade Federal do Rio de Janeiro; Brasil
Fil: S. Gonçalves, Thiago. Universidad Diego Portales; Chile
Fil: Grossi, Marcos. Universidad Diego Portales; Chile
Fil: Mendes de Oliveira, Claudia Lucia. 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
-
GALAXIES: CLUSTERS: INDIVIDUAL: NGC 4382
GALAXIES: ELLIPTICAL AND LENTICULAR, CD
GALAXIES: STAR CLUSTERS: GENERAL - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/211935
Ver los metadatos del registro completo
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The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo ClusterEscudero, Carlos GabrielCortesi, AriannaFaifer, Favio RaúlSesto, Leandro AlbertoSmith Castelli, Analia VivianaJohnston, Evelyn J.Reynaldi, María VictoriaChies Santos, AnaSalinas, R.Menendez Delmetre, KarínS. Gonçalves, ThiagoGrossi, MarcosMendes de Oliveira, Claudia LuciaGALAXIES: CLUSTERS: INDIVIDUAL: NGC 4382GALAXIES: ELLIPTICAL AND LENTICULAR, CDGALAXIES: STAR CLUSTERS: GENERALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1NGC 4382 is a merger-remnant galaxy that has been classified as morphological type E2, S0, and even Sa. In this work, we performed a photometric and spectroscopic analysis of the globular cluster (GC) system of this peculiar galaxy in order to provide additional information about its history. We used a combination of photometric data in different filters, and multiobject and long-slit spectroscopic data obtained using the Gemini/GMOS instrument. The photometric analysis of the GC system, using the Gaussian Mixture Model algorithm in the colour plane, reveals a complex colour distribution within Rgal < 5 arcmin (26.1 kpc), showing four different groups: the typical blue and red subpopulations, a group with intermediate colours, and the fourth group towards even redder colours. From the spectroscopic analysis of 47 GCs, confirmed members of NGC 4382 based on radial velocities, we verified 3 of the 4 photometric groups from the analysis of their stellar populations using the ULySS code. NGC 4382 presents the classic blue (10.4 ± 2.8 Gyr, [Fe/H] = -1.48 ± 0.18 dex), and red (12.1 ± 2.3 Gyr, [Fe/H] = -0.64 ± 0.26 dex) GCs formed earlier in the lifetime of the galaxy, and a third group of young GCs (2.2 ± 0.9 Gyr; [Fe/H] = -0.05 ± 0.28 dex). Finally, analysis of long-slit data of the galaxy reveals a luminosity-weighted mean age for the stellar population of ∼2.7 Gyr, and an increasing metallicity from [Fe/H] = -0.1 to +0.2 dex in Rgal < 10 arcsec (0.87 kpc). These values, and other morphological signatures in the galaxy, are in good agreement with the younger group of GCs, indicating a common origin as a result of a recent merger.Fil: Escudero, Carlos Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. 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: Cortesi, Arianna. Universidade Federal do Rio de Janeiro; BrasilFil: Faifer, Favio Raúl. 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: Sesto, Leandro Alberto. Observatório Do Valongo; Brasil. 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: Smith Castelli, Analia Viviana. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. 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: Johnston, Evelyn J.. Universidad Diego Portales; ChileFil: Reynaldi, María Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. 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: Chies Santos, Ana. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Salinas, R.. Gemini Observatory; ChileFil: Menendez Delmetre, Karín. Universidade Federal do Rio de Janeiro; BrasilFil: S. Gonçalves, Thiago. Universidad Diego Portales; ChileFil: Grossi, Marcos. Universidad Diego Portales; ChileFil: Mendes de Oliveira, Claudia Lucia. 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, Inc2022-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/211935Escudero, Carlos Gabriel; Cortesi, Arianna; Faifer, Favio Raúl; Sesto, Leandro Alberto; Smith Castelli, Analia Viviana; et al.; The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 511; 1; 3-2022; 393-4120035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://ieeexplore.ieee.org/document/9717075info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stac021info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:30:40Zoai:ri.conicet.gov.ar:11336/211935instacron: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 10:30:41.203CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster |
| title |
The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster |
| spellingShingle |
The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster Escudero, Carlos Gabriel GALAXIES: CLUSTERS: INDIVIDUAL: NGC 4382 GALAXIES: ELLIPTICAL AND LENTICULAR, CD GALAXIES: STAR CLUSTERS: GENERAL |
| title_short |
The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster |
| title_full |
The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster |
| title_fullStr |
The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster |
| title_full_unstemmed |
The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster |
| title_sort |
The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster |
| dc.creator.none.fl_str_mv |
Escudero, Carlos Gabriel Cortesi, Arianna Faifer, Favio Raúl Sesto, Leandro Alberto Smith Castelli, Analia Viviana Johnston, Evelyn J. Reynaldi, María Victoria Chies Santos, Ana Salinas, R. Menendez Delmetre, Karín S. Gonçalves, Thiago Grossi, Marcos Mendes de Oliveira, Claudia Lucia |
| author |
Escudero, Carlos Gabriel |
| author_facet |
Escudero, Carlos Gabriel Cortesi, Arianna Faifer, Favio Raúl Sesto, Leandro Alberto Smith Castelli, Analia Viviana Johnston, Evelyn J. Reynaldi, María Victoria Chies Santos, Ana Salinas, R. Menendez Delmetre, Karín S. Gonçalves, Thiago Grossi, Marcos Mendes de Oliveira, Claudia Lucia |
| author_role |
author |
| author2 |
Cortesi, Arianna Faifer, Favio Raúl Sesto, Leandro Alberto Smith Castelli, Analia Viviana Johnston, Evelyn J. Reynaldi, María Victoria Chies Santos, Ana Salinas, R. Menendez Delmetre, Karín S. Gonçalves, Thiago Grossi, Marcos Mendes de Oliveira, Claudia Lucia |
| author2_role |
author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
GALAXIES: CLUSTERS: INDIVIDUAL: NGC 4382 GALAXIES: ELLIPTICAL AND LENTICULAR, CD GALAXIES: STAR CLUSTERS: GENERAL |
| topic |
GALAXIES: CLUSTERS: INDIVIDUAL: NGC 4382 GALAXIES: ELLIPTICAL AND LENTICULAR, CD GALAXIES: STAR CLUSTERS: GENERAL |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
NGC 4382 is a merger-remnant galaxy that has been classified as morphological type E2, S0, and even Sa. In this work, we performed a photometric and spectroscopic analysis of the globular cluster (GC) system of this peculiar galaxy in order to provide additional information about its history. We used a combination of photometric data in different filters, and multiobject and long-slit spectroscopic data obtained using the Gemini/GMOS instrument. The photometric analysis of the GC system, using the Gaussian Mixture Model algorithm in the colour plane, reveals a complex colour distribution within Rgal < 5 arcmin (26.1 kpc), showing four different groups: the typical blue and red subpopulations, a group with intermediate colours, and the fourth group towards even redder colours. From the spectroscopic analysis of 47 GCs, confirmed members of NGC 4382 based on radial velocities, we verified 3 of the 4 photometric groups from the analysis of their stellar populations using the ULySS code. NGC 4382 presents the classic blue (10.4 ± 2.8 Gyr, [Fe/H] = -1.48 ± 0.18 dex), and red (12.1 ± 2.3 Gyr, [Fe/H] = -0.64 ± 0.26 dex) GCs formed earlier in the lifetime of the galaxy, and a third group of young GCs (2.2 ± 0.9 Gyr; [Fe/H] = -0.05 ± 0.28 dex). Finally, analysis of long-slit data of the galaxy reveals a luminosity-weighted mean age for the stellar population of ∼2.7 Gyr, and an increasing metallicity from [Fe/H] = -0.1 to +0.2 dex in Rgal < 10 arcsec (0.87 kpc). These values, and other morphological signatures in the galaxy, are in good agreement with the younger group of GCs, indicating a common origin as a result of a recent merger. Fil: Escudero, Carlos Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. 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: Cortesi, Arianna. Universidade Federal do Rio de Janeiro; Brasil Fil: Faifer, Favio Raúl. 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: Sesto, Leandro Alberto. Observatório Do Valongo; Brasil. 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: Smith Castelli, Analia Viviana. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. 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: Johnston, Evelyn J.. Universidad Diego Portales; Chile Fil: Reynaldi, María Victoria. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. 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: Chies Santos, Ana. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Salinas, R.. Gemini Observatory; Chile Fil: Menendez Delmetre, Karín. Universidade Federal do Rio de Janeiro; Brasil Fil: S. Gonçalves, Thiago. Universidad Diego Portales; Chile Fil: Grossi, Marcos. Universidad Diego Portales; Chile Fil: Mendes de Oliveira, Claudia Lucia. 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 |
NGC 4382 is a merger-remnant galaxy that has been classified as morphological type E2, S0, and even Sa. In this work, we performed a photometric and spectroscopic analysis of the globular cluster (GC) system of this peculiar galaxy in order to provide additional information about its history. We used a combination of photometric data in different filters, and multiobject and long-slit spectroscopic data obtained using the Gemini/GMOS instrument. The photometric analysis of the GC system, using the Gaussian Mixture Model algorithm in the colour plane, reveals a complex colour distribution within Rgal < 5 arcmin (26.1 kpc), showing four different groups: the typical blue and red subpopulations, a group with intermediate colours, and the fourth group towards even redder colours. From the spectroscopic analysis of 47 GCs, confirmed members of NGC 4382 based on radial velocities, we verified 3 of the 4 photometric groups from the analysis of their stellar populations using the ULySS code. NGC 4382 presents the classic blue (10.4 ± 2.8 Gyr, [Fe/H] = -1.48 ± 0.18 dex), and red (12.1 ± 2.3 Gyr, [Fe/H] = -0.64 ± 0.26 dex) GCs formed earlier in the lifetime of the galaxy, and a third group of young GCs (2.2 ± 0.9 Gyr; [Fe/H] = -0.05 ± 0.28 dex). Finally, analysis of long-slit data of the galaxy reveals a luminosity-weighted mean age for the stellar population of ∼2.7 Gyr, and an increasing metallicity from [Fe/H] = -0.1 to +0.2 dex in Rgal < 10 arcsec (0.87 kpc). These values, and other morphological signatures in the galaxy, are in good agreement with the younger group of GCs, indicating a common origin as a result of a recent merger. |
| publishDate |
2022 |
| dc.date.none.fl_str_mv |
2022-03 |
| 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/11336/211935 Escudero, Carlos Gabriel; Cortesi, Arianna; Faifer, Favio Raúl; Sesto, Leandro Alberto; Smith Castelli, Analia Viviana; et al.; The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 511; 1; 3-2022; 393-412 0035-8711 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/211935 |
| identifier_str_mv |
Escudero, Carlos Gabriel; Cortesi, Arianna; Faifer, Favio Raúl; Sesto, Leandro Alberto; Smith Castelli, Analia Viviana; et al.; The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 511; 1; 3-2022; 393-412 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://ieeexplore.ieee.org/document/9717075 info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stac021 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf application/pdf application/pdf application/pdf application/pdf |
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Wiley Blackwell Publishing, Inc |
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Wiley Blackwell Publishing, Inc |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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