(a) Use the StatStar model data on page 283 and Eq. (18.14) to make a graph of log10M˙ (vertical axis) vs. log10d (horizontal axis). Use the slope of your graph to find how the mass transfer rate, M˙, depends on d.
(b) Use Eqs. (L.1) and (L.2) to show that M˙∝d4.75 near the surface, and so verify that the mass transfer rate increases rapidly with the overlap distance d of two stars. Note that your answer to part (a) will be slightly different from this because of the density-dependence of tog\_bf (the ratio of the guillotine factor to the gaunt factor) calculated in the Opacity routine.