Ultracompact dwarfs around NGC3258 in the Antlia cluster

We present the first compact stellar systems with luminosities in the range of ultracompact dwarfs (UCDs), discovered in the Antlia galaxy cluster (-10.5<M<sub>V</sub> <-11.6). The magnitude limit between UCDs and globular clusters (CGs) is discussed. By means of imaging from VLT (...

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Detalles Bibliográficos
Autores principales: Caso, Juan Pablo, Bassino, Lilia Patricia, Richtler, Tom, Smith Castelli, Analía Viviana, Faifer, Favio Raúl
Formato: Articulo
Lenguaje:Inglés
Publicado: 2013
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/85491
Aporte de:
id I19-R120-10915-85491
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: clusters: individual: Antlia
Galaxies: Dwarf
Galaxies: Individual: NGC 3258
Galaxies: photometry
Galaxies: Star clusters: General
Glaxies: Nuclei
spellingShingle Ciencias Astronómicas
Galaxies: clusters: individual: Antlia
Galaxies: Dwarf
Galaxies: Individual: NGC 3258
Galaxies: photometry
Galaxies: Star clusters: General
Glaxies: Nuclei
Caso, Juan Pablo
Bassino, Lilia Patricia
Richtler, Tom
Smith Castelli, Analía Viviana
Faifer, Favio Raúl
Ultracompact dwarfs around NGC3258 in the Antlia cluster
topic_facet Ciencias Astronómicas
Galaxies: clusters: individual: Antlia
Galaxies: Dwarf
Galaxies: Individual: NGC 3258
Galaxies: photometry
Galaxies: Star clusters: General
Glaxies: Nuclei
description We present the first compact stellar systems with luminosities in the range of ultracompact dwarfs (UCDs), discovered in the Antlia galaxy cluster (-10.5<M<sub>V</sub> <-11.6). The magnitude limit between UCDs and globular clusters (CGs) is discussed. By means of imaging from VLT (FORS1), CTIO (MOSAIC) and the Hubble Space Telescope (ACS) archive, 11 UCDs/bright GCs are selected on the basis of photometry and confirmed as Antlia members through radial velocities measured on new Gemini (GMOS) spectra. In addition, nine UCD candidates are identified taking into account properties derived from their surface brightness profiles. All of them, members and candidates, are located in the proximity of NGC3258, one of the two brightest elliptical galaxies in the cluster core. Antlia UCDs in this sample present absolute magnitudes fainter than M<sub>V</sub> ~ -11.6 mag and most of them have colours within the blue GC range, falling only two within the red GC range. Effective radii measured for the ones lying on the ACS field are in the range R<sub>eff</sub> = 3-11 pc and are similar to equivalent objects in other clusters, obtained from the literature. The UCD sample shares the same behaviour on the size-luminosity plane: a linear relation between R<sub>eff</sub> and MV is present for UCDs brighter than M<sub>V</sub>~ -10.5 to -11 mag while no trend is detected for fainter ones, that have an approximately constant Reff. The projected spatial distribution of UCDs, GCs and X-ray emission points to an ongoing merger between two Antlia groups, dominated by NGC3258 and NGC3268. Nuclei of dwarf elliptical galaxies and blue UCDs share the same locus on the colour-magnitude diagram, supporting the hypothesis that some blue UCDs may be remnants of stripped nucleated dwarfs.
format Articulo
Articulo
author Caso, Juan Pablo
Bassino, Lilia Patricia
Richtler, Tom
Smith Castelli, Analía Viviana
Faifer, Favio Raúl
author_facet Caso, Juan Pablo
Bassino, Lilia Patricia
Richtler, Tom
Smith Castelli, Analía Viviana
Faifer, Favio Raúl
author_sort Caso, Juan Pablo
title Ultracompact dwarfs around NGC3258 in the Antlia cluster
title_short Ultracompact dwarfs around NGC3258 in the Antlia cluster
title_full Ultracompact dwarfs around NGC3258 in the Antlia cluster
title_fullStr Ultracompact dwarfs around NGC3258 in the Antlia cluster
title_full_unstemmed Ultracompact dwarfs around NGC3258 in the Antlia cluster
title_sort ultracompact dwarfs around ngc3258 in the antlia cluster
publishDate 2013
url http://sedici.unlp.edu.ar/handle/10915/85491
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