The formation of massive molecular filaments and massive stars triggered by a magnetohydrodynamic shock wave
Year: 2017
Type: article
DOI: 10.1093/pasj/psx089
Institutions: National Astronomical Observatory of Japan, Nagoya University, Centre National de la Recherche Scientifique, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, CEA Paris-Saclay - Etablissement de Saclay, Astrophysique, Instrumentation et Modélisation, Hosei University, The University of Osaka
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: closed
Awards: G2328759096, G4602357228, Innovation of the “Interstellar medium” by accurate measurements of the interstellar hydrogen, Astrophysics of Interstellar Medium Dominated by Magnetic Turbulence and Cosmic Rays, Theoretical Study of Massive Star Formation Using Three Dimensional High-resolution Magnetohydrodynamics Simulations
OpenAlex ID: W2761204985
