Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-28T02:06:21.569Z Has data issue: false hasContentIssue false
  • English
  • Français

Modeling the diffuse X-ray emission of planetary nebulae with different chemical composition

Published online by Cambridge University Press:  30 August 2012

Matthias Steffen ,
Christer Sandin ,
Ralf Jacob  and
Detlef Schönberner
Matthias Steffen
Affiliation:
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
Christer Sandin
Affiliation:
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
Ralf Jacob
Affiliation:
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
Detlef Schönberner
Affiliation:
Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Based on time-dependent radiation-hydrodynamics simulations of the evolution of Planetary Nebulae (PNe), we have carried out a systematic parameter study to address the non-trivial question of how the diffuse X-ray emission of PNe with closed central cavities is expected to depend on the evolutionary state of the nebula, the mass of the central star, and the metallicity of stellar wind and circumstellar matter. We have also investigated how the model predictions depend on the treatment of thermal conduction at the interface between the central ‘hot bubble’ and the ‘cool’ inner nebula, and compare the results with recent X-ray observations. Our study includes models whose properties resemble the extreme case of PNe with Wolf-Rayet type central stars. Indeed, such models are found to produce the highest X-ray luminosities.

Keywords

planetary nebulae: generalX-rays: starsstars: windshydrodynamicsconduction
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 215 - 218
Copyright
Copyright © International Astronomical Union 2012

References

Kastner, J. H., Montez, R., Balick, B., & De Marco, O. 2008, ApJ, 672, 957 CrossRefGoogle Scholar
Kastner, J. 2009, in: Wolk, S., Fruscione, A., Swartz, D. (eds.), Chandra's First Decade of Discovery, http://cxc.harvard.edu/symposium_2009/proceedings/session_01.html#talk03 Google Scholar
Koo, B.-C. & McKee, C. F. 1992, ApJ, 338, 103 CrossRefGoogle Scholar
Schönberner, D., Jacob, R., Sandin, C., & Steffen, M. 2010, A&A, 523, A86 Google Scholar
Steffen, M., Schönberner, D., & Warmuth, A. 2008, A&A, 489, 173 Google Scholar
Zhekov, S. A. & Perinotto, M. 1996, A&A, 309, 648 Google Scholar