Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-11T02:41:41.350Z Has data issue: false hasContentIssue false
  • English
  • Français

Mid-Infrared Observations of Planetary Nebulae

Published online by Cambridge University Press:  15 December 2006

Kevin Volk ,
B. J. Hrivnak  and
Sun Kwok
Kevin Volk
Affiliation:
Gemini Observatory, 670 N. A'Ohoku Place, Hilo, Hawaii, 96720 email: kvolk@gemini.edu
B. J. Hrivnak
Affiliation:
Department of Physics and Astronomy, Valparaiso Univeristy, Valparaiso, Indiana, 46383 email: Bruce.Hrivnak@valpo.edu
Sun Kwok
Affiliation:
Faculty of Science, The University of Hong Kong, Pokfulam, Hong Kong email: 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 present the results of a small mid-infrared imaging survey of planetary nebulae. Of 21 objects observed 19 were resolved. Only in NGC 6210 was there a marked contrast between the dust morphology and the emission line morphology. For all the other objects the dust and the gas must be well mixed even in the faint lobes of bipolar objects such as Fg3, Pe1-7, and NGC 6881.

Keywords

(ISM:) planetary nebulae: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S234: Planetary Nebulae in our Galaxy and Beyond , April 2006 , pp. 535 - 536
Copyright
© 2006 International Astronomical Union