Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-12-01T01:31:51.284Z Has data issue: false hasContentIssue false
  • English
  • Français

Molecular Hydrogen Jets, Filaments, and Haloes in Planetary Nebulae

Published online by Cambridge University Press:  15 December 2006

Mei-Yan Wang ,
C. Muthumariappan  and
Sun Kwok
Mei-Yan Wang
Affiliation:
Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan emails: [email protected], [email protected]
C. Muthumariappan
Affiliation:
Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan emails: [email protected], [email protected]
Sun Kwok
Affiliation:
Department of Physics, University of Hong Kong, Hong Kong, China email: [email protected]
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 present deep H$_2$ images of planetary nebulae obtained with the CHFTIR camera of the Canada-France-Hawaii Telescope. Molecular hydrogen emissions are seen in the equatorial torus, bipolar lobes, as well as in extended haloes. Radial equatorial jets are also detected in a number of bipolar nebulae.

Keywords

planetary nebulae: generalplanetary nebulae: individual: IC 4406K3-72NGC 2346NGC 2440ISM: molecules
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S234: Planetary Nebulae in our Galaxy and Beyond , April 2006 , pp. 537 - 538
Copyright
© 2006 International Astronomical Union