These nebulosities are described as: two spherical bipolar lobes, two outer large filamentary hour-glass shaped columns, two cone shaped rays, and a planar radially expanding, elliptically shaped chakram.
A wind of ionized matter, organized in filamentary structures at distances of 114 light days from the center, is flowing outward in the direction perpendicular to the accretion disk plane.
It occurs within a plasma with an associated electric field, that causes convection of ions and electrons inward towards a central twisting filamentary axis.
