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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: mywang@asiaa.sinica.edu.tw, muthu@asiaa.sinica.edu.tw
C. Muthumariappan
Affiliation:
Institute of Astronomy and Astrophysics, Academia Sinica, Taipei, Taiwan emails: mywang@asiaa.sinica.edu.tw, muthu@asiaa.sinica.edu.tw
Sun Kwok
Affiliation:
Department of Physics, University of Hong Kong, Hong Kong, China email: sunkwok@hku.hk
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Abstract

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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