A sample of stars from the second byurakan sky survey

A brief analysis of a sample of stars from the Second Byurakan Spectroscopic Survey is given. It contains 626 objects in the range of apparent magnitudes 10.1 ≤ m(pg) ≤ 19.5 and consists mainly of white dwarfs and subdwarfs of early spectral types. Most of the objects have been classified for the first time. Their distributions with respect to stellar magnitude and spectral type are given. Translated from Astrofizika, Vol. 40, No. 4, pp. 627–631, October-December, 1997.