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We present an equilibrium statistical mechanical theory of collisionless self-gravitational systems with isotropic velocity distributions.
We evaluate the orbital evolution and several plausible origins scenarios for the mutually inclined orbits of υ And c and d. These two planets have orbital ele-ments that oscillate with large amplitud...
We study the formation of the spiral structure of barred spiral galaxies, using an $N$-body model. The evolution of this $N$-body model in the adiabatic approximation maintains a strong spiral pattern...
We compare the DARKexp differential energy distribution, N(E) \propto \exp(\phi_0-E)-1, obtained from statistical mechanical considerations, to the results of N-body simulations of dark matter halos.
We compare the DARKexp differential energy distribution, N(E) \propto \exp(\phi_0-E)-1, obtained from statistical mechanical considerations, to the results of N-body simulations of dark matter halos.
In this paper, we present the density, \rho, velocity dispersion, \sigma, and \rho/\sigma^3 profiles of isotropic systems which have the energy distribution, N(E)\propto[\exp(\phi_0-E)-1], derived in ...
We present an equilibrium statistical mechanical theory of collisionless self-gravitational systems with isotropic velocity distributions.
Although the methods and techniques have been greatly improved since the late nineteenth century, the precision on the measurement of the gravitational constant G does not exceed 1 part in 1000. Intri...
From speckle measurements to computation of the binary system orbits at the Astronomical Observatory R. M. Aller。
Galactic Orbits of Globular Clusters in a Barred Galaxy。
Orbits of Six Binary Stars     Six Binary Stars  Orbits       < 2009/6/25
Orbits of Six Binary Stars
Herbig-Haro Jets from Sources in Elliptical Orbits
Multiple stars with both inner and outer orbits observed Spectroscopically。
Dynamics of Galactic Satellites on Elongated Orbits
Observed and Intrinsic Properties of Binary Star Orbits

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