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Fig. 3

image

Top panel: grain temperature as a function of distance from the star. Lower panel: spectral energy distributions as a function of wavelength. Structures from model A3 during the maximum (red curves) and minimum (blue curves) luminosity phase. The light red and blue curves show temperature and spectra for snapshots of the atmosphere where we set a lower temperature limit of 1000 K until the magnesium-iron layer is thermally stable.

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