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"Galaxy environments" » "Galaxy environment" (Expand Search), "Galaxy environmental" (Expand Search)
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LATIS: A Sample of IGM-selected Protoclusters and Protogroups at z ∼ 2.5
Published 2025-01-01Subjects: Get full text
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LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at z ∼ 2.5
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Evidence for Environmental Effects in the z = 4.3 Protocluster Core SPT2349–56
Published 2025-01-01Subjects: “…Galaxy environments…”
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CHILES. IX. Observational and Simulated H i Content and Star Formation of Blue Galaxies in Different Cosmic Web Environments
Published 2025-01-01Subjects: Get full text
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Cosmic Filament Spin. II. Filament Spin and Its Impact on Galaxy Spin–Filament Alignment in a Cosmological Simulation
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Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
Published 2024-01-01Subjects: Get full text
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Galaxy Rest-frame UV Colors at z ∼ 2–4 with HST UVCANDELS
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A Break in the Size–Stellar Mass Relation: Evidence for Quenching and Feedback in Dwarf Galaxies
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Mining for Protoclusters at z ∼ 4 from Photometric Data Sets with Deep Learning
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Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
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The Impact of Void-finding Algorithms on Galaxy Classification
Published 2024-01-01Subjects: “…Galaxy environments…”
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No Evidence of Asymmetrically Enhanced Star Formation in Infalling Galaxies in UNIONS
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MAGAZ3NE: Evidence for Galactic Conformity in z ≳ 3 Protoclusters
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Observed Antiparallel Correlation between Spiral Galaxy and Cosmic Filament Spins
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Virgo Filaments. V. Disrupting the Baryon Cycle in the NGC 5364 Galaxy Group
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Mapping the Star Formation and H i Gas Properties of Galaxies along Large-scale Structures around the Virgo Cluster
Published 2025-01-01Subjects: “…Galaxy environments…”
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Can Active Galactic Nuclei Activity Be Enhanced by Ram Pressure Stripping?—X-Ray Perspective
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Truncations in the X-Ray Halos of Early-type Galaxies as a Tracer of Feedback and Mergers
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