Void galaxies show modestly higher star formation rates in early spirals and outer disks, lower extinction, and higher gas-fraction proxies than matched galaxies in filaments and walls, suggesting slower quenching in underdense environments.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Large-scale cosmic environment influences galaxy stellar mass and morphology beyond local companions, with void galaxies being less massive and showing distinct shape distributions.
citing papers explorer
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The CAVITY project. The spatially resolved SFR of galaxies in voids
Void galaxies show modestly higher star formation rates in early spirals and outer disks, lower extinction, and higher gas-fraction proxies than matched galaxies in filaments and walls, suggesting slower quenching in underdense environments.
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Stellar mass and morphology segregation in pairs and multiplets in the cosmic web
Large-scale cosmic environment influences galaxy stellar mass and morphology beyond local companions, with void galaxies being less massive and showing distinct shape distributions.