A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations

Documenti analoghi

• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
  di: Arjona-Galvez, Elena, et al.
  Pubblicazione: (2024)
• HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
  di: García-Bethencourt, Guacimara, et al.
  Pubblicazione: (2026)
• An accurate measure of the size of dark matter halos using the size of galaxies
  di: Vecchia, Claudio Dalla, et al.
  Pubblicazione: (2025)
• HINORA II: Testing the Existence of the Council of Giants in ΛCDM simulations
  di: Olex, Edward, et al.
  Pubblicazione: (2026)
• Fuzzy Gasoline: Cosmological hydrodynamical simulations of dwarf galaxy formation with Fuzzy Dark Matter
  di: Nori, Matteo, et al.
  Pubblicazione: (2024)