A New Library of Synthetic Spectra and Photometry for Evolved C Stars

摘要

We present a library of synthetic spectra and photometry calculated on the basis of a grid of atmosphere and wind models for carbon-rich, pulsating AGB stars. The spectra cover the range between 0.35 and 25 μm with a spectral resolution of R = 200. The corresponding photometric variations during several pulsation periods were computed for standard broadband filters in the visual and near-infrared.