  The central star of this nebula has an observed intense magnetic field and
the fast wind is no longer present, indicating that a back flow process has
probably developed. Long-slit, spatially resolved echelle spectra have been
obtained across the main body of NGC 1360 and over its system of bipolar jets.
Deep images of the knotty structures of the jets have also been obtained. The
data allow a detailed study of the structure and kinematics of this object and
the results are modeled considering the effects of a magnetic collimation
process in the development of the nebula and then switching off the fast
stellar wind to follow its evolution to its current state. The model is able to
successfully reproduce many of the key features of NGC 1360 under these
premises.
