The collisional dynamics of particulate disks

[1]  John R. Taylor,et al.  Classical mechanics , 1999, Physics, Structure, and Reality.

[2]  J. Lissauer,et al.  Nonlinear spiral density waves - Viscous damping , 1985 .

[3]  S. Tremaine,et al.  A granular flow model for dense planetary rings , 1985 .

[4]  J. Scargle,et al.  Wavy edges suggest moonlet in Encke's gap , 1985 .

[5]  J. Lissauer,et al.  Nonlinear spiral density waves: an inviscid theory , 1985 .

[6]  G. Wetherill,et al.  The range of validity of the two-body approximation in models of terrestrial planet accumulation: I. Gravitational perturbations , 1984 .

[7]  H. Salo,et al.  Numerical simulations of collisions in systems of non-identical particles , 1984 .

[8]  M. Hausman,et al.  Spiral structure and star formation. I - Formation mechanisms and mean free paths , 1984 .

[9]  R. West,et al.  The structure of Saturn's rings: Implications from the Voyager stellar occultation , 1983 .

[10]  J. Villumsen.  The vertical growth and structure of galactic disks , 1983 .

[11]  K. A. Hämeen-Anttila.  Collisions in self-gravitating clouds of planetesimals , 1983 .

[12]  H. Zebker,et al.  Particle size distributions in Saturn's rings from voyager 1 radio occultation , 1983 .

[13]  J. Lissauer,et al.  Bending waves in Saturn's rings☆ , 1983 .

[14]  S. Tremaine,et al.  Sharp edges of planetary rings , 1982, Nature.

[15]  K. A. Hämeen-Anttila.  Starn's rings and bimodality of Keplerian systems , 1982 .

[16]  Makiko Sato,et al.  Photopolarimetry from Voyager 2; Preliminary Results on Saturn, Titan, and the Rings , 1982, Science.

[17]  K. A. Hämeen-Anttila.  Quasi-equilibrium in collisional systems , 1981 .

[18]  P. Bodenheimer,et al.  On the stability of Saturn's rings , 1981 .

[19]  W. M. Kaula,et al.  A gravitational kinetic theory for planetesimals , 1980 .

[20]  L. Cowie.  On the dynamics of agglomerating ensembles of clouds. [in interstellar space , 1980 .

[21]  D. Lin,et al.  Tidal torques on accretion discs in binary systems with extreme mass ratios. , 1979 .

[22]  S. Tremaine,et al.  Towards a theory for the uranian rings , 1979, Nature.

[23]  K. A. Hämeen-Anttila.  An improved and generalized theory for the collisional evolution of Keplerian systems , 1978 .

[24]  J. Burns,et al.  The vertical structure and thickness of Saturn's rings , 1978, Nature.

[25]  S. Tremaine,et al.  The formation of the Cassini division in Saturn's rings , 1978 .

[26]  S. Tremaine,et al.  The velocity dispersion in Saturn's rings , 1978 .

[27]  F. Shu,et al.  Galactic Shocks in an Interstellar Medium with Two Stable Phases , 1971 .

[28]  A. Cook,et al.  Erratum: Rediscussion of Maxwell's ADAMS Prize Essay on the Stability of Saturn's Rings , 1966 .

[29]  P. Bhatnagar,et al.  A Model for Collision Processes in Gases. I. Small Amplitude Processes in Charged and Neutral One-Component Systems , 1954 .

[30]  J. Scalo,et al.  Continuum models for gas in disturbed galaxies. I: Model equations , 1984 .

[31]  F. Shu.  Waves in planetary rings , 1984 .

[32]  P. Bodenheimer,et al.  Collision-induced transport processes in planetary rings , 1984 .

[33]  S. Tremaine,et al.  The Variations in Eccentricity and Apse Precession Rate of a Narrow Ring Perturbed by a Close Satellite , 1983 .

[34]  G. Wetherill.  Formation of the Terrestrial Planets , 1980 .

[35]  V. Safronov,et al.  Evolution of the protoplanetary cloud and formation of the earth and the planets , 1972 .

[36]  Subrahmanyan Chandrasekhar,et al.  Principles of Stellar Dynamics , 1942 .