Preprint Article Version 1 This version is not peer-reviewed

X-ray Shaping of Planetary Nebulae

Version 1 : Received: 30 July 2018 / Approved: 1 August 2018 / Online: 1 August 2018 (12:04:48 CEST)

A peer-reviewed article of this Preprint also exists.

Guerrero, M.A. X-ray Shaping of Planetary Nebulae. Galaxies 2018, 6, 98. Guerrero, M.A. X-ray Shaping of Planetary Nebulae. Galaxies 2018, 6, 98.

Journal reference: Galaxies 2018, 6, 98
DOI: 10.3390/galaxies6030098

Abstract

The stellar winds of the central stars of planetary nebulae play an essential role in planetary nebulae shaping. In the interacting stellar winds model, the fast stellar wind injects energy and momentum which are transfered to the nebular envelope through an X-ray-emitting hot bubble. Together with other physical processes, such as the ionization of the nebular envelope, the asymmetrical mass-loss in the AGB, and the action of collimated outflows and magnetic fields, the presurized hot gas determines the expansion and evolution of planetary nebulae. \emph{Chandra} and \emph{XMM-Newton} have provided us with detailed information of this hot gas. Here in this talk I will review our current understanding of the effects of the fast stellar wind in the shaping and evolution of planetary nebulae and give some hints of the promissing future of this research.

Subject Areas

planetary nebula; X-ray; stellar evolution

Comments (0)

We encourage comments and feedback from a broad range of readers. See criteria for comments and our diversity statement.

Leave a public comment
Send a private comment to the author(s)
Views 0
Downloads 0
Comments 0
Metrics 0


×
Alerts
Notify me about updates to this article or when a peer-reviewed version is published.