All Tables

Table 1: Comparison of some observed properties of the galactic disk in the solar neighbourhood with model results.
Table 2: Solar system element abundances a and the standard error of the abundance determination $\sigma$ .
Table 3: Average abundances a of F and G stars with solar metallicity ( $\left\vert\Delta\rm[Fe/H]\right\vert<0.05$ ) and of young stars (age $\le$ 1 Gyr) from the solar neighbourhood. $\sigma _{\rm abd}$ is the accuracy of the abundance determinations from stellar spectra, $\sigma _{*}$ is the scattering of the stellar abundances around the mean. Z is the metallicity calculated from these abundances.
Table 4: Dust species considered in the model calculation.
Table 5: Characteristic quantities and numerical coefficients used for calculating grain destruction and grain growth (SiC does not form in the ISM).
Table 6: SN presolar dust fractions and corresponding derived efficiencies of dust production.
Table 7: Surface densities of different dust species at instant of Solar System formation and at the present time as predicted by the model calculation.
Table A.1: Ejected mass of dust by AGB stars for different chemistries of M-stars, S-stars and C-stars for different initial masses M_* and metallicities Z. All masses are given in Solar mass.