Binary Interactions, High-Speed Outflows and Dusty Disks during the AGB-To-PN Transition

Binary Interactions, High-Speed Outflows and Dusty Disks during the AGB-To-PN Transition

It is widely believed that the dramatic transformation of the spherical outflows of AGB stars into the extreme aspherical geometries seen during the planetary nebula (PN) phase is linked to binarity and driven by the associated production of fast jets and central disks/torii. The key to understandin...

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Bibliographic Details
Main Author: Raghvendra Sahai
Format: Article
Language:English
Published: MDPI AG 2018-09-01
Series:Galaxies
Subjects:
planetary nebulae
AGB and post-AGB stars
binarity
accretion disks
jets
mass-loss
circumstellar matter
(sub)millimeter interferometry
ultraviolet radiation, X-rays
Online Access:http://www.mdpi.com/2075-4434/6/4/102

Internet

http://www.mdpi.com/2075-4434/6/4/102

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