The secular instability of axisymmetric collisionless star clusters
The secular variations in the restricted problem - an explicit numerical approach
The secular variations in the restricted problem's sixth-order theory and stability - an explicit numerical approach
The Segmented Prony method for the analysis of non-stationary time series
The self-consistent acceleration of cosmic rays in modified shocks with Bohm-type diffusion
The Self-Consistent Model of the Be Star Envelope and the Source of the Be-star X-ray Luminosity
The self-focusing instability in the presence of density irregularities in the ionosphere
The semidegenerate configurations of a selfgravitating system of fermions.
The sensitivity of seafloor compliance to two-dimensional low-velocity anomalies
The separation velocity of emerging magnetic flux
The ShakeOut earthquake scenario: Verification of three simulation sets
The Shane-Wirtanen counts - Observer and time-dependent effects
The shape and internal structure of Mimas
The shape of a scatter-broadened image. I - Numerical simulations and physical principles.
The shape of a scattered image - Theory and numerical simulations
The shape of bars in early-type barred galaxies
The shape of pulsar radio beams
The shape of the Galaxy
The shape of the two-point correlation function - Evidence for a double power law
The short time-scale light variability of HD 153919 revisited