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20032008
most citedEstimating the Dark Halo Mass from the Relative Thickness of Stellar Disks

26 citations · 50 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph20085 cited

Anisotropic Models of Dark Halos

N. Ya. Sotnikova, S. A. Rodionov

An iterative approach is used to construct spherically symmetric equilibrium models with an anisotropic velocity distribution. The potentialities of the method have been tested on…

astro-ph200619 cited

An Iterative Method for the Construction of Equilibrium N-Body Models for Stellar Disks

S. A. Rodionov, N. Ya. Sotnikova

One widely used technique for the construction of equilibrium models of stellar disks is based on the Jeans equations and the moments of velocity distribution functions derived usi…

astro-ph200626 cited

Estimating the Dark Halo Mass from the Relative Thickness of Stellar Disks

N. Ya. Sotnikova, S. A. Rodionov

We analyze the relationship between the mass of a spherical component and the minimum possible thickness of stable stellar disks. This relationship for real galaxies allows the low…

astro-ph2005

Optimal Choice of the Softening Length and Time-Step in N-body Simulations

S. A. Rodionov, N. Ya. Sotnikova

A criterion for the choice of optimal softening length and time-step for -body simulations of a collisionless stellar system is analyzed. Plummer and Hernquist spheres…

astro-ph2003

Mechanisms of the Vertical Secular Heating of a Stellar Disk

N. Ya. Sotnikova, S. A. Rodionov

We investigate the nonlinear growth stages of bending instability in stellar disks with exponential radial density profiles.We found that the unstable modes are global (the wavelen…