The action for the Brans-Dicke-Jordan theory of gravity is $$ \\S =\int d^4x\sqrt{-g} \; \left(\frac{\phi R - \omega\frac{\partial_a\phi\partial^a\phi}{\phi}}{16\pi} + \mathcal{L}_\mathrm{M}\right). $$
The corresponding equations of motion are $$ \Box\phi = \frac{8\pi}{3+2\omega}T\\ G_{ab} = \frac{8\pi}{\phi}T_{ab}+\frac{\omega}{\phi^2} (\partial_a\phi\partial_b\phi-\frac{1}{2}g_{ab}\partial_c\phi\partial^c\phi) +\frac{1}{\phi}(\nabla_a\nabla_b\phi-g_{ab}\Box\phi) $$
where $\\G_{ab}$ is the standard Einstein tensor and $\mathcal{L}_\mathrm{M}$ is the matter Lagrangian density. It's supposed to be obvious that this reduces to general relativity in the limit of infinitely large $\omega$. How so? You may assume that the trace $\\T$ of the stress energy tensor $\\T_{ab}$ is not zero.