a) Mn/Na vs. Mn/Mg and b) Mn/Na vs. K/Li ratios among planetary bodies. The coloured curves denote the evolution of the composition of an evaporation residue calculated using eq. 35
a) Mn/Na vs. Mn/Mg and b) Mn/Na vs. K/Li ratios among planetary bodies. The coloured curves denote the evolution of the composition of an evaporation residue calculated using eq. 35
(A)–(D). Spectrally integrated flux maps for HCN on September 12 and 15 and for CH3 on September 18 and October 1. Contour intervals in each map are given in multiples
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