We present long-slit intermediate-dispersion spectroscopic observations and narrow-band direct imaging of four classical nova shells, namely TAur, HRDel, DQHer QUVul, the nova-like source CKVul. These are used to construct models their nebular remnants using morpho-kinematic modelling tool Shape reveal 3D shape. All these but CKVul can be described by prolate ellipsoidal shells with different e...