A New Library of Synthetic Spectra and Photometry for Evolved C Stars
Abstract
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.
- Publication:
-
Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time
- Pub Date:
- August 2015
- Bibcode:
- 2015ASPC..497..111E