Field/isolated lenticular galaxies with high SN values: the case of NGC 4546 and its globular cluster system

We present a photometric study of the field lenticular galaxy NGC 4546 using Gemini/GMOS imaging in g′r′i′z′. We perform a 2D image decomposition of the surface brightness distribution of the galaxy using galfit, finding that four components adequately describe it. The subtraction of this model from...

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Detalles Bibliográficos
Autores principales: Escudero, Carlos Gabriel, Faifer, Favio Raúl, Smith Castelli, Analía Viviana, Norris, Mark A., Forte, Juan Carlos
Formato: Articulo
Lenguaje:Inglés
Publicado: 2020
Materias:
cD
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/125279
Aporte de:
id I19-R120-10915-125279
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Galaxies: elliptical and lenticular
cD
Galaxies: photometry
Galaxies: star clusters: general
spellingShingle Ciencias Astronómicas
Galaxies: elliptical and lenticular
cD
Galaxies: photometry
Galaxies: star clusters: general
Escudero, Carlos Gabriel
Faifer, Favio Raúl
Smith Castelli, Analía Viviana
Norris, Mark A.
Forte, Juan Carlos
Field/isolated lenticular galaxies with high SN values: the case of NGC 4546 and its globular cluster system
topic_facet Ciencias Astronómicas
Galaxies: elliptical and lenticular
cD
Galaxies: photometry
Galaxies: star clusters: general
description We present a photometric study of the field lenticular galaxy NGC 4546 using Gemini/GMOS imaging in g′r′i′z′. We perform a 2D image decomposition of the surface brightness distribution of the galaxy using galfit, finding that four components adequately describe it. The subtraction of this model from our images and the construction of a colour map allow us to examine in great detail the asymmetric dust structures around the galactic centre. In addition, we perform a detailed analysis of the globular cluster (GC) system of NGC 4546. Using a Gaussian Mixture Model algorithm in the colour-colour plane we detected hints of multiple groups of GC candidates: the classic blue and red subpopulations, a group with intermediate colours that present a concentrated spatial distribution towards the galaxy, and an additional group towards the red end of the colour distribution. We estimate a total GC population for NGC 4546 of 390 ± 60 members and specific frequency SN = 3.3 ± 0.7, which is relatively high compared to the typical value for galaxies of similar masses and environment. We suggest that the unusual GC population substructures were possibly formed during the interaction that led to the formation of the young ultra-compact dwarf (NGC 4546-UCD1) found in this system. Finally, we estimate the distance modulus of NGC 4546 by analyzing its luminosity function, resulting in (m − M) = 30.75 ± 0.12 mag (14.1 Mpc).
format Articulo
Articulo
author Escudero, Carlos Gabriel
Faifer, Favio Raúl
Smith Castelli, Analía Viviana
Norris, Mark A.
Forte, Juan Carlos
author_facet Escudero, Carlos Gabriel
Faifer, Favio Raúl
Smith Castelli, Analía Viviana
Norris, Mark A.
Forte, Juan Carlos
author_sort Escudero, Carlos Gabriel
title Field/isolated lenticular galaxies with high SN values: the case of NGC 4546 and its globular cluster system
title_short Field/isolated lenticular galaxies with high SN values: the case of NGC 4546 and its globular cluster system
title_full Field/isolated lenticular galaxies with high SN values: the case of NGC 4546 and its globular cluster system
title_fullStr Field/isolated lenticular galaxies with high SN values: the case of NGC 4546 and its globular cluster system
title_full_unstemmed Field/isolated lenticular galaxies with high SN values: the case of NGC 4546 and its globular cluster system
title_sort field/isolated lenticular galaxies with high sn values: the case of ngc 4546 and its globular cluster system
publishDate 2020
url http://sedici.unlp.edu.ar/handle/10915/125279
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