Synthetic radii and visibilities for pulsating red giants

Autor(en)
Josef Hron, Walter Nowotny-Schipper, Susanne Höfner
Abstrakt

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(en)
Institut für Astrophysik
Externe Organisation(en)
Uppsala University
Journal
Astrophysics and Space Science
Band
286
Seiten
213-218
Anzahl der Seiten
6
ISSN
0004-640X
DOI
https://doi.org/10.1023/A:1026132212228
Publikationsdatum
2003
ÖFOS 2012
103003 Astronomie
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/d08dd2d5-fd6f-4fdf-8739-71d2e6e2db3a