Modelling pulsating red giants: Intensity profiles and visibilities
- Author(s)
- Josef Hron, Walter Nowotny-Schipper, Rita Gautschy-Loidl, Susanne Höfner, Wolfgang Galsterer
- Abstract
We briefly summarize the status of dynamic model atmospheres for carbon rich red giants and present some recent results of comparisons between synthetic spectra and observations. We then discuss synthetic intensity profiles and visibilities for such stars. In particular, the effects of atmospheric dynamics on different spectral bands and for different model parameters are studied.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Uppsala University, University of Vienna
- Pages
- 154-159
- No. of pages
- 6
- DOI
- https://doi.org/10.1117/12.551224
- Publication date
- 2004
- Austrian Fields of Science 2012
- 103003 Astronomy
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/e9f0a75a-a844-4bb1-bee4-fefedfdc250a