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A new deep imaging survey of Planetary Nebulae with known binary central stars

Published online by Cambridge University Press:  25 May 2016

S. A. Bell  and
D. L. Pollacco
S. A. Bell
Affiliation:
1Royal Greenwich Observatory, Cambridge, UK
D. L. Pollacco
Affiliation:
2Isaac Newton Group, La Palma, Canary Islands

Extract

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Binarity in central stars is often thought to be the most likely explanation for the bipolar and axisymmetric shapes seen in planetary nebulae. Theoretical computations show that low mass stellar companions — possibly even planets, merged nuclei and long period systems will also produce bipolar-shaped nebulae. As such all known short period binary central stars are expected to have an axisymmetric nebula surrounding them.

Information

Type
IV. Envelopes
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 210
Copyright
Copyright © Kluwer 1997 

References

Bond, H.E., Livio, M., 1990, Ap.J., 355, 568.CrossRefGoogle Scholar
Bond, H.E., 1995, Ann. Israel Phys. Soc., 11, 61.Google Scholar