Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-26T16:49:49.471Z Has data issue: false hasContentIssue false
  • English
  • Français

Criteria of Classification of Long Period Variables Based on their Light Curve Changes

Published online by Cambridge University Press:  12 April 2016

V.I. Marsakova
V.I. Marsakova*
Affiliation:
Astronomical Observatory, Odessa National UniversityT.G. Shevchenko Park, Odessa, 270014, Ukrainee-mail:[email protected]

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.

Some numerical parameters of long-term changes of light curves in Long Period Variables (LPVs) are obtained. Results of analysis of the sample of 53 LPVs and classification of these stars are discussed.

Type
Part 5. Mass Loss in Pulsating Stars
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 570 - 571
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Khopolov, P.N., et al. 1985, General Catalogue of Variable Stars, Vol. I-III (Moscow: Nauka)Google Scholar
Marsakova, V.l. & Andronov, I.L. 1998, Ap&SS, 257, 49 Google Scholar
Wood, P.R. & Zarro, D.M., 1981, ApJ, 247, 247.Google Scholar