A Unified Model for Bipolar Outflows from Young Stars: The Interplay of Magnetized Wide-angle Winds and Isothermal Toroids

Large-scale morphology and time evolution are investigated for the unified model of bipolar outflows outlined in Shang et al. (2006), where an outflow forms by a radially directed, wide-angle magnetized wind interacting with magnetized isothermal toroids in various quasistatic states. The primary wi...

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Veröffentlicht in:	The Astrophysical journal 2020-12, Vol.905 (2), p.116
Hauptverfasser:	Shang, Hsien, Krasnopolsky, Ruben, Liu, Chun-Fan, Wang, Liang-Yao
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Asymptotic methods Collimation Density distribution Evolution Jets Kelvin-Helmholtz instability Low mass stars Magnetic disturbances Magnetic fields Magnetohydrodynamical simulations Magnetohydrodynamics Mixing layers (fluids) Morphology Outflow Physical properties Protostars Self-similarity Star formation Stellar jets Stellar mass loss Stellar winds Stellar-interstellar interactions Toroids Vorticity Wind Young stellar objects
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