X-ray and UV Views of Hot Gas in Planetary Nebulae-Reference-Cited by-同舟云学术

X-ray and UV Views of Hot Gas in Planetary Nebulae

Published:2003 Issue: Volume:209 Page:415-424
ISSN:0074-1809
Container-title:Symposium - International Astronomical Union
language:en
Short-container-title:Symp. - Int. Astron. Union

Author:

Chu You-Hua,Guerrero Martín A.,Gruendl Robert A.

Abstract

The interior of a planetary nebula (PN) is expected to be filled with shocked fast wind from the central star. This hot gas plays the most important role in the dynamical evolution of the PN; however, its physical conditions are not well-known because useful X-ray and far-UV observations were not available until the advent of Chandra, XMM-Newton, and FUSE. This paper reviews X-ray observations of the hot gas in PN interiors and far-UV observations of the interfaces between the hot gas and the dense nebular shells.

Publisher

Cambridge University Press (CUP)

Reference34 articles.

1. X-Ray Emission from the Wind-Blown Bubble in the Planetary Nebula BD +30°3639

2. Extended X‐Ray Emission from the Planetary Nebula BD +30o3639

3. Sonneborn G. 2002, in this volume

4. Guerrero M. A. , Gruendl R. A. , & Chu Y.-H. 2002, A&A, in press; also in this volume

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