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V645 Cyg - On the structure of a YSO
Published online by Cambridge University Press: 04 August 2017
Abstract
In the CO(J=3−2) line we observe a bipolar outflow in V645 Cyg. The physical properties of the neutral flow gas and its geometry put new constraints on the structure of this YSO.
- Type
- Bipolar Flows, Jets and Protostars
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 85 - 86
- Copyright
- Copyright © Reidel 1987
References
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