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In this article, we study the magnetohydrodynamics stagnation point flow for the upper-convected Maxwell fluid with the viscous dissipation and thermal radiation effects using the Cattaneo-Christov heat flux model. The flow equations are reconstructed and the obtained set of partial differential equations is then converted into an arrangement of nonlinear, coupled O.D.E. by utilising some reasonable similarity transformations. After this, the set of O.D.E. is solved by applying shooting method. Graphs and tables describe the behavior of physical parameters.

MHD Stagnation Point Flow with Heat Transfer Past a Porous Sheet along with Viscous Dissipation and Thermal Radiation