High-mass star formation in the Large Magellanic Cloud triggered by colliding HI flows

Ähnliche Einträge

• A multi-scale molecular and atomic gas view on the HII region N113 in the Large Magellanic Cloud:Evidence for high-mass star formation triggered by supersonically-colliding HI flows
  von: Yamada, Rin I., et al.
  Veröffentlicht: (2026)
• Giant molecular clouds and their Type classification in M74: Toward understanding star formation and cloud evolution
  von: Demachi, F., et al.
  Veröffentlicht: (2023)
• Cloud-Cloud Collision: Formation of Hub-Filament Systems and Associated Gas Kinematics; Mass-collecting cone: A new signature of Cloud-Cloud Collision
  von: Maity, A. K., et al.
  Veröffentlicht: (2024)
• ACA CO(J=2-1) Mapping of the Nearest Spiral Galaxy M33. II. Exploring the Evolution of Giant Molecular Clouds
  von: Konishi, Ayu, et al.
  Veröffentlicht: (2024)
• ALMA 0.1 pc View of Molecular Clouds Associated with High-Mass Protostellar Systems in the Small Magellanic Cloud: Are Low-Metallicity Clouds Filamentary or Not?
  von: Tokuda, Kazuki, et al.
  Veröffentlicht: (2025)