Hostname: page-component-76fb5796d-zzh7m Total loading time: 0 Render date: 2024-04-25T15:16:31.386Z Has data issue: false hasContentIssue false
  • English
  • Français

A systematic study of young multipolar planetary nebulae

Published online by Cambridge University Press:  30 August 2012

Chih-Hao Hsia  and
Sun Kwok
Chih-Hao Hsia
Affiliation:
Department of Physics, The University of Hong Kong, Pokfulam Road, Hong Kong, China email: xiazh@hku.hk; sunkwok@hku.hk
Sun Kwok
Affiliation:
Department of Physics, The University of Hong Kong, Pokfulam Road, Hong Kong, China email: xiazh@hku.hk; sunkwok@hku.hk
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.

We have analyzed the HST images of ten young planetary nebulae (PNe) and found them to possess multipolar structures. Concentric arcs and 2-D rings are also found in some objects.

Keywords

planetary nebulaegeneralstars: AGB and post-AGB
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 390 - 391
Copyright
Copyright © International Astronomical Union 2012

References

Hsia, C.-H., Kwok, S., Zhang, Y., Koning, N., & Volk, K. 2010, ApJ, 725, 173 CrossRefGoogle Scholar
Kwok, S. 2010, PASA, 27, 174 CrossRefGoogle Scholar
Sahai, R. 2000, ApJ, 537, L43 CrossRefGoogle Scholar