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Mid-Infrared Observations of Planetary Nebulae

Published online by Cambridge University Press:  15 December 2006

Kevin Volk
Affiliation:
Gemini Observatory, 670 N. A'Ohoku Place, Hilo, Hawaii, 96720 email: [email protected]
B. J. Hrivnak
Affiliation:
Department of Physics and Astronomy, Valparaiso Univeristy, Valparaiso, Indiana, 46383 email: [email protected]
Sun Kwok
Affiliation:
Faculty of Science, The University of Hong Kong, Pokfulam, Hong Kong email: [email protected]
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Abstract

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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.

Type
Contributed Papers
Copyright
© 2006 International Astronomical Union