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Using H$_2$ Emission to Study the Fast Wind in Proto-Planetary Nebulae
Published online by Cambridge University Press: 15 December 2006
Abstract
We present the results of a high-resolution H$_2$ imaging and spectroscopic study of four bipolar proto-planetary nebulae: IRAS 16594–4656, Hen 3-401, Rob 22, and IRAS 17150–3224. These reveal the locations and kinematics of the H$_2$ emission and the shaping of the nebulae by their collimated fast winds.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S234: Planetary Nebulae in our Galaxy and Beyond , April 2006 , pp. 423 - 424
- Copyright
- © 2006 International Astronomical Union
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