All Tables

Table 1: Comparison between our dynamical masses and spectroscopic masses from Kudritzki et al. (2006). Observed mass-loss rates from the same paper are also listed and compared to values from the model tracks of Blöcker (1995). He 2-108 is classified as wels, the other three are non-emission-line stars.
Table 2: Blöcker track time scales: PN visibility is defined as between $\log T_{\rm eff} = 4.4$ and either a nebular age $t = 10^4~\rm yr$ or a stellar luminosity $\log L = 3.0$ , whichever occurs earlier.
Table 3: The table contains the results collected over years of planetary nebulae modelling with Torun codes. First two columns identify the object. Next five columns contain the photoionization model parameters: logarithm of stellar black-body temperature, logarithm of stellar luminosity, assumed distance, nebular outer radius and ionized mass. Columns 8 and 9 contain the derived mass-averaged expansion velocity and turbulence. Columns 10 and 11 contain values interpolated from evolutionary tracks: stellar luminosity and its mass. Column 12 contains the derived kinematic age. Last column lists reference to the publication of data.