An Introduction to Modern Astrophysics · Problem 18.31

Physical Processes in the Solar System — Carroll & Ostlie

Physics — Astrophysics · statstar-mass-transfer-rate-overlap

Problem

(a) Use the StatStar model data on page 283 and Eq. (18.14) to make a graph of log⁡10M˙\log_{10}\dot{M} (vertical axis) vs. log⁡10d\log_{10} d (horizontal axis). Use the slope of your graph to find how the mass transfer rate, M˙\dot{M}, depends on dd. (b) Use Eqs. (L.1) and (L.2) to show that M˙∝d4.75\dot{M} \propto d^{4.75} near the surface, and so verify that the mass transfer rate increases rapidly with the overlap distance dd 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.

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