All Tables

Table 1: The sample with spectral types, variable types, periods (P), luminosities ( $L_{\star }$ ), and distances (D).
Table 2: Main-beam efficiencies ( $\eta _{{\rm mb}}$ ), and main-beam FWHM: s ( $\theta _{{\rm mb}}$ ), at the frequencies of the CO lines.
Table 3: Integrated CO( $J\rightarrow J-1$ ) intensities, $\int T_{{\rm mb}}~{\rm d}v$ , in K km s^-1.
Table 4: Mass-loss rates, h-parameters, and terminal gas expansion velocities $v_{\rm {e}}$ , derived by fitting the CO line radiative transfer model to the observations.
Table 5: Results from the dust emission modelling.
Table 6: Mass-loss rates and other quantities from the dynamical model.
Table 7: The resulting change in mass-loss rate ( $\dot{M}$ ) and dust-to-gas ratio ( $\Psi$ ) when varying the input parameters in the dynamical model of RW LMi.
Table A.1: Values for the parameters in Eq. (A.1). s_J is calibrated such that Eq. (A.1) gives the mass-loss rate in $M_\odot$ yr^-1. Values are valid in the ranges 10 $^{-7} \leq \dot{M} \leq 10 ^{-5}~M_\odot$ yr^-1, $5 \leq v_{{\rm e}} \leq 20$ km s^-1, $10^{-4} \leq f_{{\rm CO}} \leq 10 ^{-3}$ .
Table B.1: Photometric flux densities in 10^-26 W m^-2 Hz^-1.
Table C.1: The difference between the integrated CO( $J\rightarrow J-1$ ) intensities from the best-fit model and the observations, in percent; $(I_{\rm {mod}}-I_{\rm {obs}})/I_{\rm {obs}}$ .