Abstract
Bipolar outflows or polar knots are rather ubiquitous phenomena. A wealth of observational data is now available on bipolar flows associated with young stellar objects or stellar formation regions (Snell, Proc. I. A. U. Symp. Nr. 115, 1987), or nuclei of active galaxies (Asseo and Sol, 1987, Phys. Rep. 148, 307).
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