The VANDELS Survey: Star formation and quenching in two over-densities at 3<z<4

The VANDELS Survey: Star formation and quenching in two over-densities at 3<z<4

Exploring galaxy evolution in dense environments, such as proto-clusters, is pivotal for understanding the mechanisms that drive star formation and the quenching of star formation. This study provides insights into how two over-densities could have impacted the physical properties, such as the star...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2024-12
Hauptverfasser: Espinoza Ortiz, M., Guaita, L., Demarco, R., Calabró, A., Pentericci, L., Castellano, M., Celeste Artale, M., Hathi, N.P., Anton Koekemoer, M., Mannucci, F., Hibon, P., McLeod, D.J., Gargiulo, A., E., Pompei
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Sprache:eng
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Zusammenfassung:Exploring galaxy evolution in dense environments, such as proto-clusters, is pivotal for understanding the mechanisms that drive star formation and the quenching of star formation. This study provides insights into how two over-densities could have impacted the physical properties, such as the star formation rate, stellar mass, morphology, and the evolution of their members, particularly members characterised by a quenching of star formation. We focus on the over-densities identified at $3
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361/202449535