Lignende værker

• Gravity or turbulence? VII. The Schmidt-Kennicutt law, the star formation efficiency, and the mass density of clusters from gravitational collapse rather than turbulent support
  af: Zamora-Aviles, Manuel, et al.
  Udgivet: (2024)
• Comparing the $M_{gas}-N_{yso}$ Relation inside a Giant Molecular Cloud
  af: Román-Zúñiga, Carlos G., et al.
  Udgivet: (2026)
• The sonic scale does not determine the core separation in turbulent molecular clouds
  af: Manuel, Zamora-Aviles, et al.
  Udgivet: (2025)
• Dynamical heating of newborn stars driven by accretion-induced orbital tightening
  af: Camacho, Vianey, et al.
  Udgivet: (2025)
• The Turbulent Support (TS) and Global Hierarchical Collapse (GHC) models for molecular clouds compared. Differences, convergence, and myths
  af: Vázquez-Semadeni, Enrique, et al.
  Udgivet: (2024)