Associations of dwarf galaxies in a ΛCDM Universe

Associations of dwarf galaxies are loose systems composed exclusively of dwarf galaxies. These systems were identified in the Local Volume for the first time more than 30 yr ago. We study these systems in the cosmological framework of the Λ cold dark matter (ΛCDM) model. We consider the Small MultiD...

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Detalles Bibliográficos
Autores principales: Yaryura, C. Yamila, Abadi, M. G., Gottlöber, Stefan, Libeskind, Noam I., Cora, Sofía Alejandra, Ruiz, Andrés N., Vega Martínez, Cristian A., Yepes, Gustavo, Behroozi, Peter
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2020
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/132493
Aporte de:
id I19-R120-10915-132493
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: dwarf
galaxies: groups: general
galaxies: kinematics and dynamics
spellingShingle Astronomía
galaxies: dwarf
galaxies: groups: general
galaxies: kinematics and dynamics
Yaryura, C. Yamila
Abadi, M. G.
Gottlöber, Stefan
Libeskind, Noam I.
Cora, Sofía Alejandra
Ruiz, Andrés N.
Vega Martínez, Cristian A.
Yepes, Gustavo
Behroozi, Peter
Associations of dwarf galaxies in a ΛCDM Universe
topic_facet Astronomía
galaxies: dwarf
galaxies: groups: general
galaxies: kinematics and dynamics
description Associations of dwarf galaxies are loose systems composed exclusively of dwarf galaxies. These systems were identified in the Local Volume for the first time more than 30 yr ago. We study these systems in the cosmological framework of the Λ cold dark matter (ΛCDM) model. We consider the Small MultiDark Planck simulation and populate its dark matter haloes by applying the semi-analytic model of galaxy formation SAG. We identify galaxy systems using a friends-of-friends algorithm with a linking length equal to b=0.4Mpch−1 to reproduce the size of dwarf galaxy associations detected in the Local Volume. Our samples of dwarf systems are built up removing those systems that have one or more galaxies with stellar mass larger than a maximum threshold Mmax. We analyse three different samples defined by log10(Mmax[M⊙h−1])=8.5,9.0⁠, and 9.5. On average, our systems have typical sizes of ∼0.2Mpch−1⁠, velocity dispersion of ∼30kms−1⁠, and estimated total mass of ∼1011M⊙h−1⁠. Such large typical sizes suggest that individual members of a given dwarf association reside in different dark matter haloes and are generally not substructures of any other halo. Indeed, in more than 90 per cent of our dwarf systems their individual members inhabit different dark matter haloes, while only in the remaining 10 per cent members do reside in the same halo. Our results indicate that the ΛCDM model can naturally reproduce the existence and properties of dwarf galaxies’ associations without much difficulty.
format Articulo
Preprint
author Yaryura, C. Yamila
Abadi, M. G.
Gottlöber, Stefan
Libeskind, Noam I.
Cora, Sofía Alejandra
Ruiz, Andrés N.
Vega Martínez, Cristian A.
Yepes, Gustavo
Behroozi, Peter
author_facet Yaryura, C. Yamila
Abadi, M. G.
Gottlöber, Stefan
Libeskind, Noam I.
Cora, Sofía Alejandra
Ruiz, Andrés N.
Vega Martínez, Cristian A.
Yepes, Gustavo
Behroozi, Peter
author_sort Yaryura, C. Yamila
title Associations of dwarf galaxies in a ΛCDM Universe
title_short Associations of dwarf galaxies in a ΛCDM Universe
title_full Associations of dwarf galaxies in a ΛCDM Universe
title_fullStr Associations of dwarf galaxies in a ΛCDM Universe
title_full_unstemmed Associations of dwarf galaxies in a ΛCDM Universe
title_sort associations of dwarf galaxies in a λcdm universe
publishDate 2020
url http://sedici.unlp.edu.ar/handle/10915/132493
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