What boost galaxy mergers in two massive galaxy protoclusters at z = 2.24?
Characterizing the structural properties of galaxies in high-redshift protoclusters is key to our understanding of the environmental effects on galaxy evolution in the early stages of galaxy and structure formation. In this study, we assess the structural properties of 85 and 87 Hα emission-line candidates (HAEs) in the densest regions of two
Liu, Shuang et al.
Fecha de publicación:
8
2023