@inproceedings{39ef8c8c95a1455da0f8f5371e355fa9,
title = "Post-common envelope PN, fundamental or irrelevant?",
abstract = "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 = "binaries (including multiple): close, hydrodynamics, planetary nebulae: general, stars: AGB and post-AGB, stars: evolution, stars: statistics",
author = "{De Marco}, Orsola and T. Reichardt and R. Iaconi and T. Hillwig and Jacoby, {G. H.} and D. Keller and Izzard, {R. G.} and J. Nordhaus and Blackman, {E. G.}",
year = "2017",
doi = "10.1017/S1743921317002149",
language = "English",
isbn = "9781107169913",
series = "IAU symposium",
publisher = "Cambridge University Press (CUP)",
number = "323",
pages = "213--217",
editor = "Xiaowei Liu and Letizia Stanghellini and Amanda Karakas",
booktitle = "Planetary nebulae : multi-wavelength probes of stellar and galactic evolution",
address = "United Kingdom",
note = "323rd symposium of the International Astronomical Union ; Conference date: 10-10-2016 Through 14-10-2016",
}