Search for the optical variability of DC dwarfs on time scales of 0.0000005 to 40 SEC

Details Search for the optical variability of DC dwarfs on time scales of 0.0000005 to 40 SEC Search for the optical variability of DC dwarfs on time scales of 0.0000005 to 40 SEC

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..337s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, April 1989, p. 337-345. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

2

Black Holes (Astronomy), Variable Stars, White Dwarf Stars, Brightness Distribution, Continuous Spectra, Ubv Spectra

Scientific paper

The paper presents results of a search for the ultrarapid variability of DC dwarfs carried out with the 6-m telescope of the Special Astrophysical Observatory of the USSR Academy of Sciences in the framework of the MANIA experiment. The upper limits of the relative power of the variable component on the time scale of 0.0000005 to 40 sec are estimated to range from 50 to 2 percent. It is concluded that it is highly likely that there are no single black holes among the objects observed.

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