All Tables

Table 1: Collection of those WR123 models with periods around 0.5 days. The first five columns show the values of the initial hydrostatic models. Note that ${T}_{\rm eff}$ and $R_{\rm p}$ refer to model structures devoid of a wind. Starting with the sixth column, results of the non-linear computations are given such as the period P in days, the relative changes of the photospheric radius $R_{\rm p}$ , the velocity difference at the photosphere in km s^-1; the last column lists the bolometric amplitudes in magnitudes as achieved in the limit cycles.