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The Growth of Galaxy Stellar Haloes over 0.2 ≤ z ≤ 1.1

Galaxies are predicted to assemble their stellar haloes through the accretion of stellar material from interactions with their cosmic environment. Observations that trace stellar halo buildup probe the processes that drive galaxy size and stellar mass growth. We investigate stellar halo assembly ove...

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Autori principali: Devin J. Williams, Ivana Damjanov, Marcin Sawicki, Harrison Souchereau, Lingjian Chen, Guillaume Desprez, Angelo George, Marianna Annunziatella, Stéphane Arnouts, Stephen Gwyn, Danilo Marchesini, Anna Sajina
Natura: Artigo
Lingua:Inglês
Pubblicazione: IOP Publishing 2025-01-01
Serie:The Astrophysical Journal
Soggetti:
Galaxy evolution
Galaxy photometry
Galaxy interactions
Galaxy mergers
Galaxy stellar halos
Galaxy structure
Accesso online:https://doi.org/10.3847/1538-4357/ade9a8
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