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Post-common envelope PN, fundamental or irrelevant?

Published online by Cambridge University Press:  08 August 2017

Orsola De Marco ,
T. Reichardt ,
R. Iaconi ,
T. Hillwig ,
G. H. Jacoby ,
D. Keller ,
R. G. Izzard ,
J. Nordhaus  and
E. G. Blackman
Orsola De Marco
Affiliation:
Department of Physics & Astronomy, Macquarie University, Sydney, NSW 2109, Australia email: [email protected] Astronomy, Astrophysics and Astrophotonics Research Centre, Macquarie University
T. Reichardt
Affiliation:
Department of Physics & Astronomy, Macquarie University, Sydney, NSW 2109, Australia email: [email protected] Astronomy, Astrophysics and Astrophotonics Research Centre, Macquarie University
R. Iaconi
Affiliation:
Department of Physics & Astronomy, Macquarie University, Sydney, NSW 2109, Australia email: [email protected] Astronomy, Astrophysics and Astrophotonics Research Centre, Macquarie University
T. Hillwig
Affiliation:
Department of Physics & Astronomy, Valparaiso University, Indiana, USA
G. H. Jacoby
Affiliation:
Lowell Observatory, Flagstaff, AZ, USA
D. Keller
Affiliation:
KU Leuven, Belgium
R. G. Izzard
Affiliation:
Institute of Astronomy, Cambridge University, UK
J. Nordhaus
Affiliation:
National Technical Institute for the Deaf, Rochester Institute of Technology, NY, USA
E. G. Blackman
Affiliation:
University of Rochester, NY, USA
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Abstract

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One in 5 PN are ejected from common envelope binary interactions but Kepler results are already showing this proportion to be larger. Their properties, such as abundances can be starkly different from those of the general population, so they should be considered separately when using PN as chemical or population probes. Unfortunately post-common envelope PN cannot be discerned using only their morphologies, but this will change once we couple our new common envelope simulations with PN formation models.

Keywords

planetary nebulae: generalhydrodynamicsstars: AGB and post-AGBbinaries (including multiple): closestars: evolutionstars: statistics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S323: Planetary Nebulae: Multi-Wavelength Probes of Stellar and Galactic Evolution , October 2016 , pp. 213 - 217
Copyright
Copyright © International Astronomical Union 2017 

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