Intracluster light at the Frontier – II. The Frontier Fields Clusters

Intracluster light at the Frontier – II. The Frontier Fields Clusters

Abstract Multiwavelength deep observations are a key tool to understand the origin of the diffuse light in clusters of galaxies: the intracluster light (ICL). For this reason, we take advantage of the Hubble Frontier Fields (HFF) survey to investigate the properties of the stellar populations of the...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2018-02, Vol.474 (1), p.917-932
Hauptverfasser: Montes, Mireia, Trujillo, Ignacio
Format: Artikel
Sprache:eng
Schlagworte:
Computer simulation
Dark matter
Galactic clusters
Galaxies
Metallicity
Milky Way
Red shift
Star & galaxy formation
Stellar age
Stellar mass
Stellar populations
Stripping
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Zusammenfassung:Abstract Multiwavelength deep observations are a key tool to understand the origin of the diffuse light in clusters of galaxies: the intracluster light (ICL). For this reason, we take advantage of the Hubble Frontier Fields (HFF) survey to investigate the properties of the stellar populations of the ICL of its six massive intermediate redshift (0.3 
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stx2847