Hostname: page-component-8448b6f56d-mp689 Total loading time: 0 Render date: 2024-04-23T15:57:57.590Z Has data issue: false hasContentIssue false
  • English
  • Français

The Extended Atmosphere and Evolution of the RV Tau Star R Scuti

Published online by Cambridge University Press:  26 May 2016

M. Matsuura ,
A. A. Zijlstra ,
I. Yamamura  and
T. R. Bedding
M. Matsuura
Affiliation:
Dep. of Physics, UMIST, P.O. Box 88, Manchester M60 1QD, UK
A. A. Zijlstra
Affiliation:
Dep. of Physics, UMIST, P.O. Box 88, Manchester M60 1QD, UK
I. Yamamura
Affiliation:
ISAS, Yoshino-dai 3-1-1, Sagamihara, Kanagawa, 229-8510, Japan
T. R. Bedding
Affiliation:
School of Physics, University of Sydney 2006, Australia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We identify H2O, CO, SiO and CO2 bands in near-infrared ISO/SWS spectra of the RV Tau star R Sct. These molecules originate from an atmosphere around the photosphere. RV Tau stars are commonly considered as post-AGB stars. We argue that R Sct may be a thermal-pulsing AGB star, observed in a helium-burning phase.

Type
Part III: Planetary Nebulae in the Scheme of Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 87
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Jura, M., 1986, ApJ 309, 732 CrossRefGoogle Scholar
Kholopov, P.N., Samus, N.N., Frolov, M.S., et al., 1988, General Catalogue of Variable Stars. 4th Ed., Nauka Publishing House Google Scholar
Matsuura, M., Yamamura, I., Zijlstra, A.A., Bedding, T.R., 2002, A&A submitted Google Scholar