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Unveiling the small-scale web around galaxies with miniJPAS and DESI

We present the first statistical observational study detecting filaments in the immediate surroundings of galaxies, i.e. the local web of galaxies. Simulations predict that cold gas, the fuel for star formation, is channeled through filamentary structures into galaxies. Yet, direct observational evi...

Ausführliche Beschreibung

Gespeichert in:
Hauptverfasser: Galárraga-Espinosa Daniela, Kauffmann Guinevere, Bonoli Silvia, Lucie-Smith Luisa, González Delgado Rosa M., Tempel Elmo, Abramo Raul, Gurung-López Siddharta, Marra Valerio, Alcaniz Jailson, Benitez Narciso, Carneiro Saulo, Cenarro Javier, Cristóbal-Hornillos David, Dupke Renato, Ederoclite Alessandro, Hernán-Caballero Antonio, Hernández-Monteagudo Carlos, López-Sanjuan Carlos, Marín-Franch Antonio, Mendes de Oliveira Claudia, Moles Mariano, Sodré Laerte, Taylor Keith, Varela Jesús, Vázquez Ramió Hector
Format: Artigo
Sprache:Inglês
Veröffentlicht: EDP Sciences 2026-02-01
Schriftenreihe:Astronomy & Astrophysics
Schlagworte:
methods: data analysis
methods: statistical
galaxies: evolution
galaxies: fundamental parameters
galaxies: star formation
large-scale structure of universe
Online-Zugang:https://www.aanda.org/articles/aa/full_html/2026/02/aa56021-25/aa56021-25.html
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