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On the tidal interaction between protoplanets and the primordial solar nebula. II - Self-consistent nonlinear interactionA method to analyze the full nonlinear response and physical processes associated with the tidal interaction between a binary system and a thin disk in the steady state is presented. Using this approach, density wave propagation, induced by tidal interaction, may be studied for a wide range of sound speeds and viscosities. The effect of self-gravity may also be incorporated. The results of several calculations relevant to the tidal interaction between a protoplanet and the primordial solar nebula are also presented.
Document ID
19870023916
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lin, D. N. C.
(Toronto, University Canada; California, University, Santa Cruz, United States)
Papaloizou, J.
(Toronto, University Canada; Queen Mary College, London, United Kingdom)
Date Acquired
August 13, 2013
Publication Date
August 1, 1986
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 307
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
87A11190
Funding Number(s)
CONTRACT_GRANT: NSF AST-81-00163
CONTRACT_GRANT: NSF AST-83-01229
Distribution Limits
Public
Copyright
Other

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