title: An interacting binary system powers precessing outflows of an evolved star.
abstract: Stars are generally spherical, yet their gaseous envelopes often appear nonspherical when ejected near the end of their lives. This quirk is most notable during the planetary nebula phase, when these envelopes become ionized. Interactions among stars in a binary system are suspected to cause the asymmetry. In particular, a precessing accretion disk around a companion is believed to launch point-symmetric jets, as seen in the prototype Fleming 1. Our finding of a post-common-envelope binary nucleus in Fleming 1 confirms that this scenario is highly favorable. Similar binary interactions are therefore likely to explain these kinds of outflows in a large variety of systems.
authors.affiliation: European Southern Observatory (ESO), Casilla 19001, Santiago, Chile. hboffin@eso.org
authors.forename: Henri M J
authors.initials: HM
authors.lastname: Boffin
authors.forename: Brent
authors.initials: B
authors.lastname: Miszalski
authors.forename: Thomas
authors.initials: T
authors.lastname: Rauch
authors.forename: David
authors.initials: D
authors.lastname: Jones
authors.forename: Romano L M
authors.initials: RL
authors.lastname: Corradi
authors.forename: Ralf
authors.initials: R
authors.lastname: Napiwotzki
authors.forename: Avril C
authors.initials: AC
authors.lastname: Day-Jones
authors.forename: Joachim
authors.initials: J
authors.lastname: Köppen