Fig. 3
CO line fluxes taken SPIRE (open circles), HIFI (filled squares) and PACS (crosses) are shown together with the predicted fluxes from the model which is the best fit to both ground-based observations and HIFI for WX Psc (bottom) and OH 26.5+0.6 (top). The high SPIRE flux of J = 10–9 is due to a blend with a strong H2O line.
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