Disks and jets in planetary nebulae

Noam Soker; Mario Livio

doi:10.1086/173639

Disks and jets in planetary nebulae

Noam Soker^*, Mario Livio

^*Corresponding author for this work

Physics

Research output: Contribution to journal › Article › peer-review

147 Scopus citations

Abstract

Highly collimated bipolar outflows and jets have been recently observed to be associated with some planetary nebulae. Assuming that the mechanism of jet formation requires the presence of an accretion disk, we examine the possibilities to form such disks in the case of planetary nebulae with binary nuclei. We show that at the emergence from the common envelope phase, some systems can form accretion disks. Planetary nebulae therefore form the newest addition to the classes of objects (which so far include active galactic nuclei, young stellar objects, and some X-ray binaries) which produce jets.

Original language	English
Pages (from-to)	219-224
Number of pages	6
Journal	Astrophysical Journal
Volume	421
Issue number	1
DOIs	https://doi.org/10.1086/173639
State	Published - 20 Jan 1994

Keywords

Accretion, accretion disks
ISM: jets and outflows
Planetary nebulae: general

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10.1086/173639

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