Constraining the shape of dark matter haloes using only starlight. I. A new technique and its application to the galaxy Nube

Documenti analoghi

• Application of the Eddington inversion method to constrain the dark matter halo of galaxies using only observed surface brightness profiles
  di: Almeida, Jorge Sanchez, et al.
  Pubblicazione: (2024)
• The slow evolution of dark matter halos from cusp to core naturally produces extended stellar core-like distributions
  di: Almeida, Jorge Sanchez, et al.
  Pubblicazione: (2025)
• Exploring the nature of dark matter with the extreme galaxy AGC 114905
  di: Piña, Pavel E. Mancera, et al.
  Pubblicazione: (2024)
• The stellar distribution in ultra-faint dwarf galaxies suggests deviations from the collision-less cold dark matter paradigm
  di: Almeida, Jorge Sanchez, et al.
  Pubblicazione: (2024)
• Intracluster light is a close tracer of the dark matter halo shape
  di: Fernandez, Adela, et al.
  Pubblicazione: (2026)