Abstract
Three different kinds of variable stars can be found among central stars of Planetary Nebulae. Close binary central stars change their light level because of eclipses and due to the reflection effect; some hot variables have been identified as multiperiodic pulsators (e.g. see Ciardullo & Bond 1996).
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References
Ciardullo, R., Bond, H. E., 1996, AJ 111, 2332
Handler, G., 1996, in preparation
Handler, G., Méndez, R. H., Medupe, R., et al, 1996, A&A, in press
Méndez, R. H., et al., 1996, in preparation
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© 1997 Springer Science+Business Media Dordrecht
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Handler, G. (1997). Variable Central Stars of Young Planetary Nebulae. In: Habing, H.J., Lamers, H.J.G.L.M. (eds) Planetary Nebulae. International Astronimical Union / Union Astronomique Internationale, vol 180. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5244-0_33
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DOI: https://doi.org/10.1007/978-94-011-5244-0_33
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