Central Stars of Planetary Nebulae
arXiv:1611.08454 · doi:10.1017/S1743921317000862
Abstract
In this brief invited review, I will attempt to summarise some of the key areas of interest in the study of central stars of planetary nebulae which (probably) won't be covered by other speakers' proceedings. The main focus will, inevitably, be on the subject of multiplicity, with special emphasis on recent results regarding triple central star systems as well as wide binaries which avoid a common-envelope phase. Furthermore, in light of the upcoming release of Kepler's Campaign 11 data, I will discuss a few of the prospects from that data including the unique possibility to detect merger products.
4 pages, 1 figure. Submitted to the proceedings of IAUS323: Planetary nebulae: Multiwavelength probes of stellar and galactic evolution
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- Observational Confirmation of a Link Between Common Envelope Binary Interaction and Planetary Nebula Shaping
- Identifying close binary central stars of PN with Kepler
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Cited by in corpus (6)
- Planetary nebulae that cannot be explained by binary systems
- Forming H-shaped and barrel-shaped nebulae with interacting jets
- Accounting for planet-shaped planetary nebulae
- Shaping planetary nebulae with jets in inclined triple stellar systems
- Morphologies and Central Stars of Planetary Nebulae in the Galactic bulge from VLT, and Pan-STARRS imaging
- Post-AGB nebular studies