The orion complex according to observations of the space telescope glazar G. M. TovmasyanR. Kh. OganesyanD. Huguenin OriginalPaper Pages: 155 - 162
Spectroscopic investigation of objects of the Second Byurakan Survey. Stellar objects. V Dzh. A. StepanyanV. A. LipovetskiiA. I. Shapovalova OriginalPaper Pages: 163 - 170
Strong increase of the linear polarization of RZ Psc at deep minimum N. N. KiselevN. Kh. MinikulovG. P. Chernova OriginalPaper Pages: 175 - 181
Is TZ Ori a star of RR Lyr type? É. S. ParsamyanA. S. MelkonyanG. B. Oganyan OriginalPaper Pages: 182 - 185
Polarimetric investigations of blue stellar objects of the First Byurakan Survey A. M. MikaelyanM. A. EritsyanG. V. Abramyan BriefCommunication Pages: 186 - 188
Distribution and motions of OB stars in the direction of h andχ Perseus L. V. MirzoyanV. V. AmbaryanA. T. Garibdzhanyan OriginalPaper Pages: 189 - 202
Structure of the central regions of some galaxies with ultraviolet excess. II G. V. AbramyanK. A. SaakayanÉ. E. Khachikyan BriefCommunication Pages: 203 - 205
Markaryan 907: An interacting system of galaxies A. R. PetrosyanA. N. BurenkovK. A. Saakyan OriginalPaper Pages: 206 - 211
OJ 287 in 1983: Spectral energy distribution of variable source in the optical and ultraviolet regions V. A. Gagen-TornA. I. GataullinaO. V. Mikolaichuk OriginalPaper Pages: 212 - 215
Estimate of the accuracy of depth asymptotics in some problems of radiative transfer Zh. M. DlugachÉ. G. Yanovitskii OriginalPaper Pages: 216 - 225
Maximum likelihood image restoration. VII. Wandering of image due to atmospheric turbulence and reconstruction in computerized tomography V. Yu. TerebizhO. K. CherbuninaYu. G. Cherbunin OriginalPaper Pages: 226 - 232
Maximum likelihood image restoration. IV. Limiting resolution for given alternative V. Yu. Terebizh Correction Pages: 232 - 233
Plasma model of pulsar emission and some observational consequences A. Z. KazbegiG. Z. MachabeliT. V. Smirnova OriginalPaper Pages: 234 - 242
Rotation dynamics and surface temperatures of neutron stars D. M. SedrakyanA. D. Sedrakyan OriginalPaper Pages: 243 - 247