Abstract
AbstractThe formation and evolution of dust grains following a nova outburst are reviewed, and various observational methods of constraining the nature of nova dust are described. Despite recent advances in understanding grain formation and evolution in classical nova systems, there remains a number of outstanding problems, the solutions to which are likely to come from studies of other aspects of the nova outburst.
Publisher
Cambridge University Press (CUP)
Reference46 articles.
1. Space, Stars, C
60
, and Soot
2. Matese J.J. , Whitmire D.P. & Reynolds R.T. , 1989. In IAU Symposium 135 Interstellar Dust, in press.
3. Formation of silicon carbide particles behind shock waves
4. Hyland A.R. & McGregor P.J. , 1989. In IAU Symposium 135 Interstellar Dust, in press.
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