Synthetic radii and visibilities for pulsating red giants

Author(s)
Josef Hron, Walter Nowotny-Schipper, Susanne Höfner
Abstract

We present synthetic radii and visibilities in the IR, based on hydrostatic and dynamic model atmospheres of carbon stars. The differences between these two sets of input models and to uniform disc models are discussed and compared to the expected capabilities of the VLTI.

Organisation(s)
Department of Astrophysics
External organisation(s)
Uppsala University
Journal
Astrophysics and Space Science
Volume
286
Pages
213-218
No. of pages
6
ISSN
0004-640X
DOI
https://doi.org/10.1023/A:1026132212228
Publication date
2003
Austrian Fields of Science 2012
103003 Astronomy
Portal url
https://ucrisportal.univie.ac.at/en/publications/d08dd2d5-fd6f-4fdf-8739-71d2e6e2db3a