Relation between colour gradient and central asymmetric features for post-starburst galaxies at $z \sim 0.8$

Documenti analoghi

• Evolution of the early-type fraction in massive galaxies at $z<2$: how did early-type morphology form?
  di: Kajisawa, Masaru
  Pubblicazione: (2026)
• Gas excitation of post-starburst galaxies at 0.6 < z < 1.3
  di: Zanella, A., et al.
  Pubblicazione: (2025)
• Gas-phase metallicity gradients in galaxies at $z \sim 6-8$
  di: Venturi, G., et al.
  Pubblicazione: (2024)
• The importance of gas starvation in driving satellite quenching in galaxy groups at $z\sim 0.8$
  di: Baxter, Devontae C., et al.
  Pubblicazione: (2024)
• TP-AGB stars and stellar population properties of a post-starburst galaxy at $z \sim 2$ through optical and NIR spectroscopy with JWST
  di: Bevacqua, Davide, et al.
  Pubblicazione: (2025)