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Molecular envelopes of young and proto PNe
Published online by Cambridge University Press: 25 May 2016
Abstract
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I review recent results of mm-wave interferometric observations of molecular envelopes of young and proto planetary nebulae. Spatial resolutions of mm-wave interferometers now reach from one to a few arcseconds; together with line observations reveale very small structures in molecular envelopes of planetary nebulae. These small scale structures are probably caused by an instability of the radiation-driven, gas-dust outflow. Implications of these observations and theories are discussed.
- Type
- IV. Envelopes
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- Copyright
- Copyright © Kluwer 1997
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