All Tables

Table 1: Selected models along the evolutionary track of a $3~M_\odot$ Pop I star. The filtered angular momentum luminosity ${\cal L}_{\rm J}^{\rm fil}$ is taken as 0.05 R below the CZ (or at $R_{\rm cz}/2$ if it is larger) for a differential rotation of $\delta \Omega = 0.001~\mu{\rm Hz}$ . Also provided are the star's moment of inertia of the radiative zone $I_{\rm R}$ and the resulting timescale $\tau =I_{\rm R} \delta \Omega /{\cal L}_{\rm J}^{\rm fil}$ for IGWs. The last column gives the time $\Delta t$ between consecutive models (with the convention $\Delta t_i = t_{i+1} - t_i$ ). No waves are generated in models 4 to 11.