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A (microns)

Fig. 7.21 Sensitivity of the synthetic spectrum of a Pegasid to the presence of TiO and VO. These two theoretical spectra of a Pegasid, calculated by Hubeny et al. (2003), show the profound alterations caused by the presence of visible and UV absorbers (here TiO and VO) in the profile of the overall spectrum, from the UV to the thermal infrared (Burrows et al., 2006)

7.3 The Atmospheres of Exoplanets: Their Structure, Evolution and Spectral Characteristics 227 Ne Ar Kr Xe

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