Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-28T05:28:57.607Z Has data issue: false hasContentIssue false

On the Possible Relationship Between the Photometric Parameters of the AGB Stars and Their Evolutionary Status

Published online by Cambridge University Press:  07 August 2017

L.S. Kudashkina
Affiliation:
Department of Astronomy, Odessa State University, T.G. Shevchenko Park, Odessa 270014 Ukraine
I.L. Andronov
Affiliation:
Department of Astronomy, Odessa State University, T.G. Shevchenko Park, Odessa 270014 Ukraine

Extract

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.

The statistical study of the Long-Period Variables, provided by various authors, show, that there is a relationship between the photometric characteristics and the physical properties. For example, the asymmetry of the light curve may be related with the strength of the shock wave. The presence of the maser-fed line emission characterizes the definite evolutionary stage of the Long-Period Variable.

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Copyright
Copyright © Kluwer 1993