Hydrodynamical Simulations of Jet- and Wind-driven Protostellar Outflows
arXiv:astro-ph/0104373 · doi:10.1086/321648
Abstract
We present two-dimensional hydrodynamical simulations of both jet- and wind-driven models for protostellar outflows in order to make detailed comparisons to the kinematics of observed molecular outflows. Comparing the different simulations with observations, we find that some outflows, e.g., HH 212, show features consistent with the jet-driven model, while others, e.g., VLA 05487, are consistent with the wind-driven model.
38 pages, 14 figures, accepted for publication in ApJ
Cited by in corpus (87)
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