A statistical approach for interpreting polarized dust emission of the filamentary molecular clouds toward the estimate of 3D magnetic field structure

Documenti analoghi

• Formation of unipolar outflow and $\textit{protostellar rocket effect}$ in magnetized turbulent molecular cloud cores
  di: Takaishi, Daisuke, et al.
  Pubblicazione: (2024)
• Ion-Neutral Drift Velocity as a Diagnostic of Dust Growth and Magnetic Field in Star-Forming Environments
  di: Fukihara, Haruka, et al.
  Pubblicazione: (2026)
• Co-evolution of dust grains and protoplanetary disks II: structure and evolution of protoplanetary disks; an analytical approach
  di: Tsukamoto, Yusuke
  Pubblicazione: (2024)
• Probing the filamentary nature of star formation in the California giant molecular cloud
  di: Zhang, Guo-Yin, et al.
  Pubblicazione: (2024)
• Development of 1-D non-ideal MHD simulation code towards understanding Long-term Evolution of Protoplanetary Disk
  di: Kobayashi, Yudai, et al.
  Pubblicazione: (2025)