The excitation of water in the S140 photon dominated region

We consider the excitation of water in the Photon Dominated Region (PDR) S140. With the use of a three-dimensional escape probability method we compute the level populations of ortho- and para-H(2)O up to similar to 350 K ( i. e., 8 levels), as well as line intensities for various transitions. Homogeneous and inhomogeneous models are presented with densities of 10(4)-10(5) cm(-3) and the differences between the resulting intensities are displayed. Density, temperature, and abundance distributions inside the cloud are computed with the use of a self-consistent physi-chemical (in) homogeneous model in order to reproduce the line intensities observed with SWAS, and to make predictions for various lines that HIFI will probe in the future. Line intensities vary from similar to 10(-13) erg cm(-2) s(-1) sr(-1) to a few times 10(-6) erg cm(-2) s(-1) sr(-1). We can reproduce the intensity for the 1(10) -> 1(01) line observed by the SWAS satellite. It is found that the 2(12) -> 1(01) line is the strongest, whereas the 3(12) -> 2(21) line is the weakest, in all the models. It is found that the 1(10) -> 1(01) line probes the total column, while higher excitation lines probe the higher density gas ( e. g., clumps).