Maximum likelihood image restoration. III. Algorithm. One-dimensional test problems

Crimean Laboratory of the P. K. Shternberg State Astronomical Institute. Translated from Astrofizika, Vol. 33, No. 2, pp. 305–315, September–October, 1990.     

Pulsar radio emission. II. Inclined rotator

A new mechanism of production of pulsar radio emission is suggested. An equation for pulsar radio luminosity is derived for the case of an inclined rotator.Translated from Astrofizika, Vol. 39, No. 3, pp. 489–514, July–September, 1996.     

Two-color photometry of clusters of galaxies. III. A2256

Osservatorio Astronomico di Roma; Byurakan Astrophysical Observatory. Published in English in Astrofizika, Vol. 29, No. 2, pp. 232–246, September–October, 1988.     

Gravitating configurations with magnetic field. III. Dedekind and Riemann ellipsoids

Kiev Polytechnic Institute. Translated from Astrofizika, Vol. 30, No. 1, pp. 208–219, January–February, 1989.     

First Byurakan Spectral Sky Survey. Blue stellar objects. VI. Zone +33°≤δ≤+37°

Byurakan Astrophysical Observatory. Translated fromAstrofizika, Vol. 36, No. 4, pp. 517–526, October–December, 1993.     

UBV photometry of Seyfert galaxies. II. NGC 6814

P. K. Shternberg State Astronomical Institute. Translated from Astrofizika, Vol. 28, No. 2, pp. 233–242, March–April, 1988.     

Maximum likelihood image restoration. II. Point and line spread functions

P. K. Shternberg State Astronomical Institute. Translated from Astrofizika, Vol. 33, No. 1, pp. 113–127, July–August, 1990.     

Pear-shaped figures of equilibrium with internal motion. I. The two-dimensional case

Pedagogical Institute, Glazov. Translated from Astrofizika, Vol. 32, No. 3, pp. 471–489, May–June, 1990.     

Heating of gas in stellar flares. I. Heating by protons

Crimean Astrophysical Observatory; Leningrad State University. Translated from Astrofizika, Vol. 31, No. 3, pp. 527–537, November–December, 1989.     

Compact radio sources as plasma turbulent reactors. III. Accretion model

Erevan State University. Translated from Astrofizika, Vol. 32, No. 2, pp. 341–353, March–April, 1990.     

Spectroscopic investigations of objects of the Second Byurakan Survey. Stellar objects. IV

Byurakan Astrophysical Observatory; Special Astrophysical Observatory, USSR Academy of Sciences. Translated from Astrofizika, Vol. 34, No. 1, pp. 5–12, January–February, 1991.     

Dynamics of a special spheroidal model of homogeneous stellar systems. I. Steady states

Pedagogical Institute, Glazov. Translated from Astrofizika, Vol. 31, No. 2, pp. 369–387, September–October, 1989.     

Spectroscopic investigation of objects of the Second Byurakan Survey. Stellar objects. V

Byurakan Astrophysical Observatory; Special Astrophysical Observatory. Translated from Astrofizika, Vol. 34, No. 3, pp. 315–325, May–June, 1991.     

Investigation of light curves of young irregular variables. 1. SV Cep and CQ Tau

Institute of Astrophysics, Academy of Sciences of Tadzhikistan. Shternberg State Astronomical Institute. Odessa Observatory. Translated from Astrofizika, Vol. 36, No. 1, pp. 55–60, January–February, 1993.     

Statistical investigation of flare stars. III. Flare stars in the general galactic star field

Byurakan Astrophysical Observatory. Translated from Astrofizika, Vol. 29, No. 3, pp. 531–540, November–December, 1988.     

Equilibrium configurations of protomatter. II

Byurakan Astrophysical Observatory. Translated from Astrofizika, Vol. 33, No. 1, pp. 143–153, July–August, 1990.     

Scalar-tensor bimetric theory of gravitation. II. Energy-momentum tensor of the gravitational field

Institute of Applied Physics Problems, Armenian Academy of Sciences. Translated from Astrofizika, Vol. 33, No. 1, pp. 107–112, July–August, 1990.     

Modeling of convective motions in the envelope of procyon. II. Asymmetry of the spectral lines

Principal Astronomical Observatory, Ukrainian Academy of Sciences. Translated from Astrofizika, Vol. 31, No. 3, pp. 589–600, November–December, 1989.     

UBV photometry of Seyfert galaxies. I. MCG 8-11-11 and Markaryan 6

P. K. Shternberg State Astronomical Institute. Translated from Astrofizika, Vol. 28, No. 1, pp. 5–17, January–February, 1988.     

Abundances of elements of the palladium group in the atmospheres of evolved stars. I. Molybdenum

Principal Astronomical Observatory, Ukrainian Academy of Sciences. Translated from Astrofizika, Vol. 28, No. 3, pp. 595–598, May–June, 1988.