Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-30T03:42:15.468Z Has data issue: false hasContentIssue false
  • English
  • Français

Comparison of C-Rich Mira, Semiregular, and Irregular Variables

Published online by Cambridge University Press:  25 May 2016

Franz Kerschbaum ,
Peter Habison ,
Rita Loidl ,
Hans Olofsson  and
Josef Hron
Franz Kerschbaum
Affiliation:
Institut für Astronomie der Universität Wien, Vienna, Austria
Peter Habison
Affiliation:
Institut für Astronomie der Universität Wien, Vienna, Austria Kuffner-Sternwarte, Vienna, Austria
Rita Loidl
Affiliation:
Institut für Astronomie der Universität Wien, Vienna, Austria
Hans Olofsson
Affiliation:
Stockholms Observatorium, Saltsjöbaden, Sweden
Josef Hron
Affiliation:
Institut für Astronomie der Universität Wien, Vienna, Austria

Abstract

An abstract is not available for this content so a preview has been provided. As you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Abstracts of Posters
Information
Symposium - International Astronomical Union , Volume 177: The Carbon Star Phenomenon , 2000 , pp. 547
Copyright
Copyright © Kluwer 2000