Lyman-alpha Radiation Pressure in Dense Star Clusters: Implications for Star Formation and Winds at Cosmic Dawn

Documenti analoghi

• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
  di: Andalman, Zachary Lee, et al.
  Pubblicazione: (2024)
• Lyman-$α$ feedback prevails at Cosmic Dawn: Implications for the first galaxies, stars, and star clusters
  di: Nebrin, Olof, et al.
  Pubblicazione: (2024)
• Primordial Rotating Disk Composed of $\geq$15 Dense Star-Forming Clumps at Cosmic Dawn
  di: Fujimoto, S., et al.
  Pubblicazione: (2024)
• The Interplay between the IMF and Star Formation Efficiency through Radiative Feedback at High Stellar Surface Densities
  di: Menon, Shyam H., et al.
  Pubblicazione: (2024)
• Hot Jupiter Formation in Dense Star Clusters
  di: Benkendorff, Leonard, et al.
  Pubblicazione: (2024)