PLANETARY NEBULAE: THEIR EVOLUTION AND ROLE IN THE UNIVERSE

By Q. Parker, M. Hartley, D. Russeil, A. Acker, F. Ochsenbein, D. Morgan, S. Beaulieu, R. Morris, Steve Phillipps, Martin Cohen. 2003

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The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars (2014, result): “This fraction is close to the fraction of bipolar PNe found by Manchado (2003), at 17%.”
Preplanetary Nebulae: A Hubble Space Telescope Imaging Survey and a New Morphological Classification System (2007, methodology): “A detailed morphological classification of the young PNs from the HST surveys described in Sahai & Trauger (1998) and Sahai (2003), which are presumably most closely related to PPNs in an evolutionary sense, will be presented in a future paper (Sahai & Morris 2007, in preparation).”
The Origin and Shaping of Planetary Nebulae: Putting the Binary Hypothesis to the Test (2009, background): “A similar match is reached for K 1-2, where similar binary central star and PN inclinations have been determined by Exter et al. (2003) and Corradi et al. (1999), respectively.”
s-Process Nucleosynthesis in Asymptotic Giant Branch Stars: A Test for Stellar Evolution (2002, background): “The alternative mixing process related to rotation may limit the neutron flux by continued mixing of 14N into the s-process layer during the interpulse phase (Herwig et al. 2002).”