Fig. 5
Spectral energy distribution of W Hya. The included Photometry is not corrected for reddening effects and the black body curve is only included for guidance. The ISO LWS and SWS spectra from observation epochs 1996-02-07 and 1992-02-14 are used, respectively. The MIDI spectrum (green, where light green are the errors) does not show the silicate emission feature at around 10 microns. The MIDI spectrum is shown in the inset in more detail.
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