Physics
Scientist
Inst. Kosmicheskoj Astronomii
Erevanskii Politekhnicheskii Institut, Yerevan, Armenian SSR
Atomic data for pseudoresonance lines of A1 II and Si II. Interpretation of the short-wavelength spectrum of AU Mon
Broad absorption lines in the spectra of planetary nebulae as indicators of fast flows.
Determination of the temperatures of the central stars of planetary nebulas
Luminosity function of the cluster of galaxies A2634
Method of determinig the distance of a planetary nebula using pseudoresonance lines
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