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

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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Bibliographic Details
Main Authors: 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
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Galaxy evolution
Galaxy photometry
Galaxy interactions
Galaxy mergers
Galaxy stellar halos
Galaxy structure
Online Access:https://doi.org/10.3847/1538-4357/ade9a8
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https://doi.org/10.3847/1538-4357/ade9a8

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