All Tables

Table 1: Parameter values of the standard model.
Table 2: Adopted Ba ( $Y_{{\rm Ba}}(m)$ ) and Eu ( $Y_{{\rm Eu}}(m)$ ) yields and ejected r-process matter ( $M_{\rm r}$ ) as function of progenitor mass m of models SN810, SN2025 and SN2050. Yields in the mass range 8- $10 ~ {M}_{\odot}$ are assumed to be constant (SN810). Yields in the mass range 20- $25 ~ {M}_{\odot}$ are linearly interpolated (SN2025). Yields of model SN2050 exhibit a more complex behaviour: a rapid decline in the mass range 20- $28 ~ {M}_{\odot}$ is assumed. Progenitors with masses 28- $50 ~ {M}_{\odot}$ all have the same, constant yield.
Table 3: Constraints on the Galactic NSM rate $f_{{\rm NSM}}$ and ejected r-process matter $M_{\rm r}$ .
Table 4: Parameter values adopted for NSM events (see text for details). For each value of $P_{\rm NSM}$ , two models with the indicated coalescence timescales $t_{\rm c}$ have been calculated.