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We present the preliminary results of the first 3-dimensional (3D)Morpho-Kinematical (MK) model of a supernova remnant (SNR), using as a studycase the Galactic SNR VRO 42.05.01 (G 166.0+4.3). For the purpose of ourmodelling, the astrophysical software SHAPE was employed in which wide fieldimaging and high resolution spectroscopic data were utilized. We found that theremnant is consisted by three basic distinctive components: a "shell", a "wing"and a "hat", which present different morphological and kinematical behaviour,probably due to different ambient medium properties. The whole nebula has aninclination of $6-8$ degrees with respect to the plane of the sky and asystemic velocity $V_{\rm sys}$ $\sim$ -15 to -25 km/s. Finally, we discuss thepossible implications of our model's results on the origin and evolution of VRO42.05.01.

The first 3D Morpho-kinematical model of a Supernova Remnant: The case of VRO 42.05.01 (G 166.0+4.3)