The metal-poorest tail of the Galactic halo: hypothesis on its origin from precise spectral analysis

Documenti analoghi

• The intrinsic dispersion of elemental abundance ratios in nearby metal-poor halo stars
  di: Nissen, Poul Erik, et al.
  Pubblicazione: (2026)
• The earliest phases of CNO enrichment in galaxies
  di: Rossi, Martina, et al.
  Pubblicazione: (2024)
• Barium isotopic ratios in metal-poor stars: calibrating the method with globular clusters
  di: Giribaldi, Riano E., et al.
  Pubblicazione: (2025)
• How homogeneous was the chemical enrichment of the Milky Way 13 gigayears ago?
  di: Giribaldi, Riano E., et al.
  Pubblicazione: (2025)
• Extended Drag-Based Model for better predicting the evolution of Coronal Mass Ejections
  di: Rossi, Mattia, et al.
  Pubblicazione: (2024)