Galaxy mass-size segregation in the cosmic web from the CAVITY parent sample

Context. The mass-size relation is a fundamental galaxy scaling relation that is intrinsically linked to galaxy formation and evolution. The physical processes involved in galaxy growth leave their particular imprint on the relation between the stellar or total mass and galaxy size.

Bibliographic Details
Authors: Pérez, I., Gil, L., Ferré-Mateu, A., Torres-Ríos, Gloria, Zurita, A., Argudo-Fernández, María, Bidaran, B., Sánchez-Menguiano, L., Ruiz-Lara, T., Domínguez-Gómez, J., Duarte Puertas, S., Espada, Daniel, Falcón-Barroso, J., García-Benito, Rubén, Jiménez, A, Peletier, R. F., Román, J., Sánchez Alarcón, P., Sánchez-Blázquez, Pilar, Vásquez-Bustos, P.
Format: article
Status:Published version
Publication Date:2025
Country:España
Institution:Consejo Superior de Investigaciones Científicas (CSIC)
Repository:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/385527
Online Access:http://hdl.handle.net/10261/385527
Access Level:Open access
Keyword:Galaxies: evolution
Galaxies: formation
Large-scale structure of Universe
Description
Summary:Context. The mass-size relation is a fundamental galaxy scaling relation that is intrinsically linked to galaxy formation and evolution. The physical processes involved in galaxy growth leave their particular imprint on the relation between the stellar or total mass and galaxy size.

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