No CrossRef data available.
Article contents
Dust formation in C-star shells
Published online by Cambridge University Press: 04 August 2017
Abstract
The formation of carbon grains is described by a chemical pathway from acetylene via polyaromatic hydrogens (PAHs). The proposed mechanism is in excellent agreement with the observations and provides in particular the observed low condensation temperature which cannot be explained by classical nucleation theory.
- Type
- Circumstellar Dust and Chemistry
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 543 - 544
- Copyright
- Copyright © Reidel 1987