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- W2686476852 endingPage "1049" @default.
- W2686476852 startingPage "1026" @default.
- W2686476852 abstract "The relation between the mass accretion rate onto the circumstellar disc and the rate of mass ejection by magnetically driven winds is investigated using three-dimensional magnetohydrodynamics simulations. Using a spherical cloud core with a varying ratio of thermal to gravitational energy, which determines the mass accretion rate onto the disc, to define the initial conditions, the outflow propagation for approximately 10^4 yr after protostar formation is then calculated for several cloud cores. The mass ejection rate and accretion rate are comparable only when the magnetic energy of the initial cloud core is comparable to the gravitational energy. Consequently, in strongly magnetised clouds a higher mass accretion rate naturally produces both massive protostars and massive outflows. The simulated outflow mass, momentum, kinetic energy and momentum flux agree well with observations, indicating that massive stars form through the same mechanism as low-mass stars but require a significantly strong magnetic field to launch massive outflows." @default.
- W2686476852 created "2017-06-30" @default.
- W2686476852 creator A5038429764 @default.
- W2686476852 creator A5051175770 @default.
- W2686476852 creator A5076114483 @default.
- W2686476852 creator A5088685130 @default.
- W2686476852 date "2017-06-24" @default.
- W2686476852 modified "2023-10-14" @default.
- W2686476852 title "Massive outflows driven by magnetic effects in star-forming clouds with high mass accretion rates" @default.
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