Synthetic polarization observations of magnetized pillars in HII regions: The limitations of the Davis-Chandrasekhar-Fermi method

Documents similaires

• The sonic scale does not determine the core separation in turbulent molecular clouds
  par: Manuel, Zamora-Aviles, et autres
  Publié: (2025)
• 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
  par: Zamora-Aviles, Manuel, et autres
  Publié: (2024)
• Comparing the $M_{gas}-N_{yso}$ Relation inside a Giant Molecular Cloud
  par: Román-Zúñiga, Carlos G., et autres
  Publié: (2026)
• Gravity or turbulence? VI. The physics behind the Kennicutt-Schmidt relations
  par: Ballesteros-Paredes, Javier, et autres
  Publié: (2024)
• The Turbulent Support (TS) and Global Hierarchical Collapse (GHC) models for molecular clouds compared. Differences, convergence, and myths
  par: Vázquez-Semadeni, Enrique, et autres
  Publié: (2024)