Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since $z = 12$

Documenti analoghi

• The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies
  di: Nadolny, Jakub, et al.
  Pubblicazione: (2024)
• Atomic gas properties at the positions of supernovae Type Ia, II, and Ib/c
  di: Šlaus, Bruno, et al.
  Pubblicazione: (2026)
• The Fate of the Interstellar Medium in Early-type Galaxies. V. AGN Feedback from Optical Spectral Classification
  di: Ryzhov, Oleh, et al.
  Pubblicazione: (2024)
• The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation
  di: Michałowski, Michał J., et al.
  Pubblicazione: (2024)
• Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6
  di: Koprowski, M. P., et al.
  Pubblicazione: (2025)