A multi-wavelength investigation of spiral structures in $z > 1$ galaxies with JWST

Documenti analoghi

• Galactic bars are already mature at Cosmic Noon: bar strength and flatness at z ~ 1.5
  di: Kalita, Boris S., et al.
  Pubblicazione: (2025)
• Gas Fraction and Depletion Time Drive the Main-Sequence Scatter in Massive Galaxies at $z\sim1.5$
  di: Kashino, Daichi, et al.
  Pubblicazione: (2026)
• A PAH deficit in the starburst core of a distant spiral galaxy
  di: Liu, Zhaoxuan, et al.
  Pubblicazione: (2025)
• Clumps as multiscale structures in cosmic noon galaxies
  di: Kalita, Boris S, et al.
  Pubblicazione: (2025)
• JWST and ALMA discern the assembly of structural and obscured components in a high-redshift starburst galaxy
  di: Liu, Zhaoxuan, et al.
  Pubblicazione: (2023)