Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-24T22:30:07.605Z Has data issue: false hasContentIssue false
  • English
  • Français

Chaotic Behavior and Statistical Analysis of Some Mira and Sr Stars

Published online by Cambridge University Press:  12 April 2016

T. Yanagita ,
H. Satoh  and
K. Saijo
T. Yanagita
Affiliation:
The Institute of Statistical Mathematics, 4-6-7 Minami-Azabu, Minato-ku. Tokyo 106, Japan
H. Satoh
Affiliation:
Institute of Astronomy, The University of Tokyo, Mitaka, Tokyo 181, Japan
K. Saijo
Affiliation:
Department of Science and Engineering, National Science Museum, Ueno Park, Taitou-ku, Tokyo 110, Japan

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.

Visual light curves of some Mira and semiregular variable stars are analyzed to search for their chaotic and statistical behaviour. Discussion are also given.

Type
II. Observational Facts
Information
International Astronomical Union Colloquium , Volume 134: Nonlinear Phenomena in Stellar Variability , 1993 , pp. 149 - 151
Copyright
Copyright © Kluwer 1993

References

Akaike, H. and Nakagawa, T.: 1988, Statistical Analysis and Control of Dynamic Systems (Kluwer Academic Pub).Google Scholar
Grassberger, P. and Procaccia, I.: 1983, Physical Review Letters 50, 346.Google Scholar
Kholopov, P.N. (ed.): 1985, General Catalogue of Variable Stars. 4th edition (Astronomical Council of USSR Academy of Science, Moscow).Google Scholar
Saijo, K. and Kiyota, S.: 1991, Bull. Natn. Sci. Mus., Ser. E. 14, 11.Google Scholar
Wood, P.R.: 1975, in Multiple Periodic Variable Stars, ed. Fitch, W.S., IAU Colloq., 29, 69.Google Scholar