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The leonid meteor swarm in 2000-2002 the astronomers to improve its orbital elements. The simulation of a meteoroid swarm on the basis of the new
The influence of meteoric radiant and velocity distribution on the reflection-region characteristics in oblique radar sounding be explained only in terms of the astronomical model based on the concept of microstreams. © 1998 MAHK Hayka
Comparative analysis of meteor shower observations processed by three different methods observations worked out at the Engelhardt Astronomical Observatory.
On the systems of selenographic coordinates, their determination and terminology astronomical time service on the Moon. Since the future expeditions to the Moon will be able to keep
Dwarf nova EZ Lyncis second visit to instability strip© 2014 © The Author 2014. Published by Oxford University Press on behalf of the Astronomical
Investigation of Cyg OB2 #11(O5 Ifc) by modelling its atmosphere, which did not reveal any. © 2014 Astronomical Society of Australia.
Discovery of the Sub-second Linearly Polarized Spikes of Synchrotron Origin in the UV Ceti Giant Optical FlareCopyright © Astronomical Society of Australia 2017During our optical monitoring of UV Ceti, iconic
New calibrations for abundance determinations in HII regions© 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical
Oxygen abundance maps of CALIFA galaxies© 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical
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