Structure and evolution of nearby stars with planets. I. Short-period systems

Using the Yale stellar evolution code, we have calculated theoretical model s for nearby stars with planetary-mass companions in short-period nearly ci rcular orbits: 51 Pegasi, tau Bootis, upsilon Andromedae, rho(1) Cancri, an d rho Coronae Borealis. We present tables listing key stellar parameters su ch as mass, radius, age, and size of the convective envelope as a function of the observable parameters (luminosity, effective temperature, and metall icity), as well as the unknown helium fraction. For each star we construct best models based on recently published spectroscopic data and the present understanding of galactic chemical evolution. We discuss our results in the context of planet formation theory and, in particular, tidal dissipation e ffects and stellar metallicity enhancements.