All Tables

Table 1: Multiplicities $\omega$ of the 13 inequivalent atoms of C₃₂H₁₄ labelled in Fig. 2 and corresponding statistical weigth, evaluated from the probabilities of p^*=0.631 and q^*=0.002 for ¹²C and H to be replaced by their most aboundant isotopes ¹³C and D, respectively.
Table 2: Numerical values of the predicted ratios between ${\rm d}F_{\rm obs}/{\rm d}\Omega$ (for the two far-infrared skeletal vibrational modes at about 85 and 150 $\mu$ m) and $\mathcal{W}_{\rm DIB}$ of the electronic transition near 9701 Å of C₃₂H₁₄⁺, as obtained through our simulation in the four different radiation fields considered. The ratios in the table are expressed in units of W cm^-2 sr^-1 mÅ^-1.
Table 3: Values of $\mathcal{P}$ , as defined in Sect. 3, for C₃₂H₁₄ without isotopic substitutions; bands with a fraction of emitted photons below 0.1% were omitted, leaving 52 out of the 56 IR-active modes of C₃₂H₁₄ (cf. Table 5 in mal03c).
Table 4: Values of $\mathcal{P}$ , as defined in Sect. 3, for C₃₂H₁₄⁺ without isotopic substitutions; bands with a fraction of emitted photons below 0.1% were omitted, leaving 53 out of the 56 IR-active modes of C₃₂H₁₄⁺ (cf. Table 6 in mal03c).