Tracing the assembly history of NGC 1395 through its Globular Cluster System

We used deep Gemini-South/GMOS g'r'i'z' images to study the globular cluster (GC) system of the massive elliptical galaxy NGC1395, located in the Eridanus supergroup. The photometric analysis of the GC candidates reveals a clear colour bimodality distribution, indicating the pres...

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Autores principales: Escudero, Carlos Gabriel, Faifer, Favio Raúl, Smith Castelli, Analía Viviana, Forte, Juan Carlos, Sesto, Leandro Alberto, González, Nélida Mabel, Scalia, María Cecilia
Formato: Articulo
Lenguaje:Inglés
Publicado: 2018
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/94046
https://academic.oup.com/mnras/article-abstract/474/4/4302/4662636?redirectedFrom=fulltext
Aporte de:
id I19-R120-10915-94046
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Astronomía
Galaxies: clusters: individual: NGC 1395
Galaxies: elliptical and lenticular, cD
Galaxies: evolution
spellingShingle Astronomía
Galaxies: clusters: individual: NGC 1395
Galaxies: elliptical and lenticular, cD
Galaxies: evolution
Escudero, Carlos Gabriel
Faifer, Favio Raúl
Smith Castelli, Analía Viviana
Forte, Juan Carlos
Sesto, Leandro Alberto
González, Nélida Mabel
Scalia, María Cecilia
Tracing the assembly history of NGC 1395 through its Globular Cluster System
topic_facet Astronomía
Galaxies: clusters: individual: NGC 1395
Galaxies: elliptical and lenticular, cD
Galaxies: evolution
description We used deep Gemini-South/GMOS g'r'i'z' images to study the globular cluster (GC) system of the massive elliptical galaxy NGC1395, located in the Eridanus supergroup. The photometric analysis of the GC candidates reveals a clear colour bimodality distribution, indicating the presence of 'blue' and 'red' GC subpopulations. While a negative radial colour gradient is detected in the projected spatial distribution of the red GCs, the blue GCs display a shallow colour gradient. The blue GCs also display a remarkable shallow and extended surface density profile, suggesting a significant accretion of low-mass satellites in the outer halo of the galaxy. In addition, the slope of the projected spatial distribution of the blue GCs in the outer regions of the galaxy, is similar to that of the X-ray halo emission. Integrating up to 165 kpc the profile of the projected spatial distribution of the GCs, we estimated a total GC population and specific frequency of 6000 ± 1100 and S N = 7.4 ± 1.4, respectively. Regarding NGC1395 itself, the analysis of the deep Gemini/GMOS images shows a low surface brightness umbrella-like structure indicating, at least, one recent merger event. Through relations recently published in the literature, we obtained global parameters, such as M stellar = 9.32 × 10 11 M⊙ and M h = 6.46 × 10 13 M⊙. Using public spectroscopic data, we derive stellar population parameters of the central region of the galaxy by the full spectral fitting technique. We have found that this region seems to be dominated for an old stellar population, in contrast to findings of young stellar populations from the literature.
format Articulo
Articulo
author Escudero, Carlos Gabriel
Faifer, Favio Raúl
Smith Castelli, Analía Viviana
Forte, Juan Carlos
Sesto, Leandro Alberto
González, Nélida Mabel
Scalia, María Cecilia
author_facet Escudero, Carlos Gabriel
Faifer, Favio Raúl
Smith Castelli, Analía Viviana
Forte, Juan Carlos
Sesto, Leandro Alberto
González, Nélida Mabel
Scalia, María Cecilia
author_sort Escudero, Carlos Gabriel
title Tracing the assembly history of NGC 1395 through its Globular Cluster System
title_short Tracing the assembly history of NGC 1395 through its Globular Cluster System
title_full Tracing the assembly history of NGC 1395 through its Globular Cluster System
title_fullStr Tracing the assembly history of NGC 1395 through its Globular Cluster System
title_full_unstemmed Tracing the assembly history of NGC 1395 through its Globular Cluster System
title_sort tracing the assembly history of ngc 1395 through its globular cluster system
publishDate 2018
url http://sedici.unlp.edu.ar/handle/10915/94046
https://academic.oup.com/mnras/article-abstract/474/4/4302/4662636?redirectedFrom=fulltext
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