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

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

2001-10-23

arxiv.org/abs/astro-ph/0110505v1

Astronomy and Astrophysics

Astrophysics

To appear in ASP Conference Series, proceedings of ``Observed HR diagrams and stellar evolution: the interplay between observa

Scientific paper

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 our work, by comparing our predictions for the AGB
star R Fornacis with the results of Lorenz-Martins & Lefevre (1994) based on
the dust spectral energy distribution.

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