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Model atmospheres with periodic shocksThe pulsation of a long-period variable star generates shock waves which dramatically affect the structure of the star's atmosphere and produce conditions that lead to rapid mass loss. Numerical modeling of atmospheres with periodic shocks is being pursued to study the processes involved and the evolutionary consequences for the stars. It is characteristic of these complex dynamical systems that most effects result from the interaction of various time-dependent processes.
Document ID
19900044163
Document Type
Conference Paper
Authors
Bowen, G. H.
(Iowa State University of Science and Technology, Ames, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Subject Category
Astrophysics
Meeting Information
Meeting: IAU Colloquium
Location: Bloomington, IN
Country: United States
Start Date: July 27, 1988
End Date: July 29, 1988
Accession Number
90A31218
Funding Number(s)
CONTRACT_GRANT: NAGW-1364
CONTRACT_GRANT: NAG5-707
Distribution Limits
Public
Copyright
Other

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