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OH 231.8+4.2: its energetic bipolar outflow and rich chemistry
Published online by Cambridge University Press: 25 May 2016
Abstract
We report results from observations taken at different wavelengths (optical, radio and NIR) of the bipolar Protoplanetary Nebula OH 231.8+4.2. Radio interferometry with high spatial resolution has been particularly revealing. We study the complex structure and dynamics of this object as well as its rich chemistry.
- Type
- Part 4. Circumstellar Envelopes
- Information
- Symposium - International Astronomical Union , Volume 191: Asymptotic Giant Branch Stars , 1999 , pp. 347 - 352
- Copyright
- Copyright © Astronomical Society of the Pacific 1999