Azreg-Ninou, MustaphaHaroon, SumarnaJamil, MubasherRizwan, Muhammed2021-02-252021-02-2520190218-2718http://hdl.handle.net/11727/5405Depending on five parameters, rotating counterparts of Einstein-Maxwell-dilaton black holes are derived. We discuss their physical and geometric properties and investigate their null and timelike geodesics including circular orbits. The Lense-Thirring effect is considered.enginfo:eu-repo/semantics/closedAccessEinstein-Maxwell-dilaton theoryrotating solutionsgeodesic motionLense-Thirring effectRotating normal and phantom Einstein-Maxwell-dilaton black holes: Geodesic analysisarticle2840004609255000072-s2.0-85059613948