We derive the spatial variations of dust continuum emission at
different wavenumbers, which are compared with those of the [O III] 88 micron (113 cm ^ -1) emission and the OH 119 micron (84 cm ^ -1) absorption.
Phil says: «Where do you get your value of 0.2 emissivity from, what range of
wavenumber is it for, why haven't you accounted for the variation of energy over the
wavenumber range or the
different absorption bands of H2O and CO2?»