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- W4253181947 abstract "There is strong evidence for magnetic fields in molecular clouds to be oriented parallel to the direction of bipolar outflows. We have evidence for Alfvén waves in molecular clouds from the facts that: (i) the velocity width of CO lines, ΔV, is approximately twice the gravitational energy, and (ii) polarization maps indicate well-defined magnetic fields. These facts indicate that ΔV is wave-like and not eddy-like. We study the Alfvén wave protostellar model of Jatenco-Pereira and Opher (1989) to explain the observed bipolar outflows and turbulence in molecular clouds. We assume that the Alfvén waves are primarily dissipated by non-linear damping and examine the physical parameters necessary to produce the observed massive low-velocity bipolar outflows (u ∞ ∿ 10 − 50 km s −1 and Ṁ ∿ 10 −3 M ⊙ yr −1 ) and turbulence in molecular clouds." @default.
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- W4253181947 date "1992-01-01" @default.
- W4253181947 modified "2023-09-24" @default.
- W4253181947 title "Bipolar Outflow and Turbulence in Molecular Clouds Due to Protostellar Alfvén Waves" @default.
- W4253181947 cites W1963492294 @default.
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- W4253181947 doi "https://doi.org/10.1017/s0074180900090513" @default.
- W4253181947 hasPublicationYear "1992" @default.
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