Into the Modelling of RU Vir

Autor(en)
G. Rau, J. Hron, C. Paladini, Kjell Eriksson, B. Aringer, M. A. T. Groenewegen, Marko Mecina
Abstrakt

We present an attempt to model the atmosphere of the carbon-rich Mira star RU Vir, using different techniques including spectroscopy, photometry, and interferometry. A radiative transfer code and hydrostatic model atmospheres were used for a preliminary study. To investigate the dynamic processes happening in RU Vir, dynamic model atmospheres were compared to new MIDI/VLTI observations obtained in April 2014, and SiC opacities were added.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Uppsala University
Seiten
137 - 138
Publikationsdatum
08-2015
ÖFOS 2012
103004 Astrophysik, 103003 Astronomie
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/into-the-modelling-of-ru-vir(22792a64-0fbc-439f-85aa-9faa507e72b7).html