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Astron. Astrophys. Suppl. Ser. 140, 287-292

Binary star speckle measurements during 1992-1997 from the SAO 6-m and 1-m telescopes in Zelenchuk

I.I. Balega - Y.Y. Balega - A.F. Maksimov - E.A. Pluzhnik - Z.U. Shkhagosheva - V.A. Vasyuk

Send offprint request: Y.Y. Balega,

Special Astrophysical Observatory of the Russian Academy of Science Nizhnij Arkhyz 357147, Russia

Received August 18; accepted September 3, 1999


We present the results of speckle interferometric measurements of binary stars made with the television photon-counting camera at the 6-m Big Azimuthal Telescope (BTA) and 1-m telescope of the Special Astrophysical Observatory (SAO) between August 1992 and May 1997. The data contain 89 observations of 62 star systems on the large telescope and 21 on the smaller one. For the 6-m aperture 18 systems remained unresolved. The measured angular separation ranged from 39 mas, two times above the BTA diffraction limit, to 1593 mas.

Key words: stars: binaries: visual -- techniques interferometric -- catalogs

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