The physics of double layers and their role in astrophysics
The Picard iterative approximation to the solution of the integral equation of radiative transfer. II. Three-dimensional geometry.
The Piecewise Parabolic Method (PPM) for Gas-Dynamical Simulations
The planet vanishes
The planetary bunches formation modeling from a dust-gas protoplanetary cloud
The planning and analysis of galactic disk tracer observations
The plasma jet in M87 - Energy balance and the spectral index
The plasma mechanism of IR emission of X-ray pulsars
The point spread function of silicon pore x-ray optics
The polarization of radiation from hot stars
The polarization of the microwave background in open universes
The possibility of electron detection from the decay of solar neutrons
The possibility of investigating turbulence in distant objects on the basis of the emission spectrum of cosmic electrons
The possibility of negative diffusion in a compressible turbulent medium
The possible effect of oscillations on results of observations of the first neutrino burst from SN 1987A
The potential for supernova-induced chemical enrichment of protoglobular cluster clouds
The Potential of Non-standard Pulsation Models for Asteroseismology
The power spectra of dark halos in a cold dark matter universe
The power spectrum of galaxy clustering
The power-law galaxies