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Paper: Magneto-Hydrodynamical Models of the Knotty, Collimated Jet in Hen 2-90
Volume: 313, Asymmetrical Planetary Nebulae III
Page: 465
Authors: Lee, C.-F.; Sahai, R.
Abstract: A remarkably linear, bipolar, knotty jet was recently discovered in Hen 2-90, an object classified as a young planetary nebula (PN). Using two-dimensional magneto-hydrodynamical simulations, we investigate periodic variations in jet density and velocity as the mechanism for producing the jet and its knotty structures. From a detailed comparison between the Hα emission derived from our models to the observations, we find that a non-magnetized jet with density or velocity variations does not reproduce in detail the observed structure of the Hen 2-90 jet -- a magnetized jet with periodic velocity variations is required.
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