All Tables

Table 1: Input parameters for the adopted, spherically symmetric model nebula (CLOUDY)
Table 2: Four-step model-PN evolution. Integrated intensity of representative nebular emissions (relative to I(H $\beta )=100$ ), absolute H $\beta$ flux, and ionized mass for the adopted, spherically symmetric nebula (Table 1) powered by a hydrogen-burning post-AGB star of 0.605 $M_\odot$ .