Computer Science – Sound
Scientific paper
Aug 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...307..395l&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 307, Aug. 1, 1986, p. 395-409. NASA-supported research.
Computer Science
Sound
106
Nebulae, Planetary Evolution, Protoplanets, Solar Corona, Solar Planetary Interactions, Tides, Accretion Disks, Density Distribution, Difference Equations, Pressure Effects, Self Consistent Fields, Shock Waves, Viscosity
Scientific paper
The authors present a 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. 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 authors present the results of several calculations relevant to the tidal interaction between a protoplanet and the primordial solar nebula.
Lin Doug N. C.
Papaloizou John
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