A system of OB stars in the Carina nebula

Byurakan Astrophysical Observatory and Geneva Observatory. Translated from Astrofizika, Vol. 36, No. 1, pp. 35–54, January–Feburary, 1993.     

Nature of the variability of the subfour V 1143 Ori

Byurakan Astrophysical Observatory; Tonantzintla Observatory, Mexico. Translated from Astrofizika, Vol. 34, No. 2, pp. 175–180, March–April, 1991.     

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.     

Flares of H2O maser radio line in the sources GDD 25 and Sgr B2

Special Astrophysical Observatory, USSR Academy of Sciences; Byurakan Astrophysical Observatory. Translated from Astrofizika, Vol. 30, No. 1, pp. 121–127, January–February, 1989.     

The orion complex according to observations of the space telescope glazar

Byurakan Astrophysical Observatory; Geneva Observatory. Translated from Astrofizika, Vol. 34, No. 3, pp. 301–314, May–June, 1991.     

Markaryan 907: An interacting system of galaxies

Byurakan Astrophysical Observatory; Special Astrophysical Observatory, USSR Academy of Sciences. Translated from Astrofizika, Vol. 34, No. 3, pp. 383–394, May–June, 1991.     

Spectral investigations of stellar objects from the second Byurakan sky survey. I. The fields centered on α=08h00m, δ=+59°00′ and α=09h47m, δ=+51°00′

Byurakan Astrophysical Observatory; Special Astrophysical Observatory, USSR Academy of Sciences. Translated from Astrofizika, Vol. 33, No. 1, pp. 89–105, July–August, 1990.     

Spectroscopic investigations of stellar objects from the Second Byurakan Sky Survey. II. The fields centered on α=09h50m, δ=+55°00′ and α=11h30m, δ=+59°00′

Byurakan Astrophysical Observatory; Special Astrophysical Observatory, USSR Academy of Sciences. Translated from Astrofizika, Vol. 33, No. 2, pp. 199–212, September–October, 1990.     

Forbidden lines in the spectrum of P Cyg

Byurakan Astrophysical Observatory; Armagh Observatory (Northern Ireland). Translated from Astrofizika, Vol. 34, No. 3, pp. 327–332, May–June, 1991.     

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.     

Stars of early types in the region of the Orion Stellar association OB1 from observations of the glazar space telescope

Byurakan Astrophysical Observatory; SKB Granit; Geneva Observatory; Cosmonaut Preparation Center. Translated from Astrofizika, Vol. 32, No. 2, pp. 197–202, March–April, 1990.     

Connection between the magnetic field strengths and the helium abundance in helium-rich stars

Special Astrophysical Observatory, USSR Academy of Sciences; Crimean Astrophysical Observatory, USSR Academy of Sciences. Translated from Astrofizika, Vol. 33, No. 3, pp. 363–370, November–December, 1990.     

Spectrophotometric investigation of the galaxy Markaryan 7

Special Astrophysical Observatory, USSR Academy of Sciences; Byurakan Astrophysical Observatory. Translated from Astrofizika, Vol. 32, No. 2, pp. 245–254, March–April, 1990.     

Observations of the compact group of galaxies Shahbazian 130

Byurakan Astrophysical Observatory and Special Astrophysical Observatory, Academy of Sciences. Translated fromAstrofizika, Vol. 35, No. 1, pp. 67–75, July–August, 1991.     

Detailed morphological and spectrophotometric investigation of the galaxy Markaryan 1118

Special Astrophysical Observatory, USSR Academy of Sciences; Byurakan Astrophysical Observatory. Translated from Astrofizika, Vol. 29, No. 2, pp. 223–231, September–October, 1988.     

Slit spectra of galaxies of the Second Byurakan Survey. III

Special Astrophysical Observatory, USSR Academy of Sciences; Byurakan Astrophysical Observatory. Translated from Astrofizika, Vol. 29, No. 3, pp. 548–555, November–December, 1988.     

Analysis of the molecular spectra of N stars on the basis of model atmospheres

Byurakan Astrophysical Observatory; Principal Astronomical Observatory, Ukrainian Academy of Sciences. Translated from Astrofizika, Vol. 30, No. 2, pp. 249–258, March–April, 1989.     

V1589 Cyg=B19: A foreground dMe flare star in the direction of NGC 7000

Institute of theoretical Astrophysics, Oslo, Norway; Department of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences; Department of Astronomy and McDonald Observatory, Austin, Texas, USA; Department of Physics and Astronomy, University of Arkansas at Little Rock, Arkansas, USA; Byurakan Astrophysical Observatory Armenian Academy of Sciences, USSR. Published in English in Astrofizika, Vol. 19, No. 1, 67–73, July–August, 1988.     

At the 2.6 m telescope of Byurakan Perot-Fabry observations of gas emission in nebulae with cigale

During the summer of 1985, the CIGALE Perot-Fabry scanning interferometer of Marseilles Observatory was installed at the prime focus of the 2.6 m telescope of Byurakan Observatory. The long run (two new moons) was successful and gave matereial for numerous publications.Published in Astrofizika, Vol. 38, No. 4, pp. 619–624, October–December, 1995.     

An atlas of coronal hole boundary positions May 28 to November 21, 1973

This atlas shows the boundary locations of the coronal holes observed in soft X-rays (2–32, 44–54 Å) by the AS & E X-ray spectrographic telescope on Skylab. The data are presented as tracings of the boundaries as they appeared when the holes were near central meridian.Center for Astrophysics - Harvard College Observatory, Smithsonian Astrophysical Observatory.