Massive outflows driven by magnetic effects – II. Comparison with observations

Abstract The driving mechanism of massive outflows observed in high-mass star-forming regions is investigated using three-dimensional magnetohydrodynamics (MHD) and protostellar evolution calculations. In our previous paper, we showed that the mass outflow rate depends strongly on the mass accretion...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2018-03, Vol.475 (1), p.391-403
Hauptverfasser:	Matsushita, Yuko, Sakurai, Yuya, Hosokawa, Takashi, Machida, Masahiro N
Format:	Artikel
Sprache:	eng
Schlagworte:	Deposition Ejection Fluid dynamics Kinetic energy Luminosity Magnetic effects Magnetic fields Magnetohydrodynamics Massive stars Momentum Outflow Protostars Simulation Star & galaxy formation Star formation Stellar evolution Stellar winds
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