Вісник астрономічної школи
- » Auroral activity in connection with structure of the heliospheric magnetic field
- » The Kunya–Urgench H5 Chondrite and its cosmophysical evidence
- » Kinetics gas phase chemical reactions during eruptions of volcanoes on Io
- » Installation for radio observations of meteors
- » Peculiarities of spectra of comet C/2002 T7 (LINEAR) in January 2004
- » Peculiarity of solar radiation scattering by dust in the head of comet...
- » Identification of emission lines in the spectrum of comet C/2002 V1 (NEAT)
- » The light curves of comets C/2000 WM1 (LINEAR), C/2001 A2 (LINEAR), C/2002 C1...
- » Photometric observations of six asteroids carried out in Simeiz in 2002
- » Shift the photometric center of the gegenschein
- » Modelling of meteors light-curves
- » A statistical modelling of meteor showers
- » The birth of the young meteor streams near the Sun
- » On dynamical and physical evolution of 95P/Chiron as Centaurs representative
- » Statistical distributions of orbital elements of interstellar meteors
- » Consideration of meteoroid rotation in physical theory of meteors
- » Physical properties of comet 81P Wild 2
- » Models of SOHO comets with near-parabolic orbits
- » The interpretation of meteor radiation
- » The use of patrol plates of the Odessa astronomical observatory for study period...
- » Spectral manifestations of the small-scale magnetic field inhomogeneity in solar flare...
- » Gamma-ray flash from relativistic shock break out at the surface of Hypernova star
- » Numerical simulations of the chemical evolution of complex gravitating disk and dwarf...
- » Methods of determination of the abundance of oxygen in HII regions. Oxygen abundance...
- » The construction of а new catalogue of galaxy clusters