Spectra of galaxies with ultraviolet continuum. VIII V. A. LipovetskiiA. I. ShapovalovaL. K. Erastova OriginalPaper Pages: 665 - 672
BVR photometry of the distant cluster of galaxies a 665 A. T. KalloglyanD. NanniA. Vignato OriginalPaper Pages: 672 - 678
Structure of the central regions of some galaxies with ultraviolet excess G. V. AbramyanK. A. Saakyan OriginalPaper Pages: 678 - 685
Results of search for ultrarapid optical variability of radio objects with continuous optical spectra V. F. ShvartsmanG. M. BeskinS. A. Pustil'nik OriginalPaper Pages: 685 - 690
Dynamics of a special spheroidal model of homogeneous stellar systems. II. Spheroidal pulsations B. P. Kondrat'ev OriginalPaper Pages: 696 - 703
CoKu Tau/1: A new object with bipolar optical outflow T. A. MovsesyanT. Yu. Magakyan OriginalPaper Pages: 711 - 714
Low dispersion spectral sky survey to find faint carbon stars. IV. Region 90°l115°, −5°≤b≤+5° O. M. KurtanidzeM. G. Nikolashvili OriginalPaper Pages: 714 - 724
On the reality of the observed chemical anomalies of Am stars in the light of their binary nature L. S. Lyubimkov OriginalPaper Pages: 725 - 729
Heating of gas in stellar flares. I. Heating by protons V. P. GrininV. V. Sobolev OriginalPaper Pages: 729 - 735
Determination of fundamental properties of giant stars by means of the Geneva photometric system L. V. KorotinaA. V. DragunovaN. S. Komarov OriginalPaper Pages: 735 - 742
Disturbance of the dipole magnetic field in the meridional plane of pulsars I. F. MalovS. A. Suleimanova OriginalPaper Pages: 742 - 749
Strong shock waves in a spherically symmetric motion of gravitating gas E. A. FilistovA. D. Chernin BriefCommunication Pages: 749 - 751
Two generations of low-mass x-ray binaries. Recycled radio pulsars G. S. Bisnovatyi-Kogan OriginalPaper Pages: 751 - 758
Corrugation instability of a strong slow parallel shock wave. II. Approximate analytic investigation M. A. Édel'man OriginalPaper Pages: 758 - 764
Modeling of convective motions in the envelope of procyon. II. Asymmetry of the spectral lines I. N. AtroshchenkoA. S. GadunR. I. Kostyk OriginalPaper Pages: 765 - 772
