Line surveys in evolved stars and their global analysis: the case of CRL 618

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Scientific paper

The aim of this presentation was to introduce the importance of C-rich Post-AGB objects as efficient factories of complex molecules in Space and how a multiwavelength approach is necessary to understand their physical conditions and chemistry. In particular, we focus on a 80-275 GHz survey of the c-rich protoplanetary nebula CRL 618, carried out with the IRAM-30m telescope, for which a global analysis has allowed us to assign more than 3000 spectral features, with less than 100 U-ines, and to actually build a 3D radiative transfer model that reproduces reasonably well the whole data set thus providing detailed information on the physics and chemistry that is going on.

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