Temperature predictions for dust embedded AGB stars: how far can we go with synthetic near-infrared photometry ?

E. Lastennet, S. Lorenz-Martins, F. Cuisinier +1

We discuss the possibilities of the BaSeL models in its lowest temperature boundary (Teff ~ 2500 K for cool giants) to provide the Teff of AGB stars. We present the first step of o…