Deval Mehta spent the summer modeling gas clouds around quasars under the guidance of Dr. Stanley Owocki. Mehta started by working on a simple one-dimensional Monte Carlo scattering model with another student. This provided background for modeling gas pressure in clouds as a function of optical depth. Mehta is using the VH1 hydrodynamics code coupled with radiation modeling to simulate a one-dimensional planar gas cloud confined by pressure on one side and radiation on the other. The goal is to achieve hydrostatic equilibrium in the cloud. Mehta plans to extend the model to two dimensions and introduce density perturbations to analyze their effects on the cloud behavior.