- as
gravity waves. It was
first reported to be
variable by
Shulov and
Kopatskaya in 1974. DAV
stars are like
normal white dwarfs but have
luminosity variations...
- Hagen-Thorn,
Vladimir A.; Joshi, Manasvita; Konstantinova,
Tatiana S.;
Kopatskaya,
Evgenia N. (2014-06-23). "Comprehensive
Monitoring of Gamma-ray Bright...
- ; Villata, M.; Raiteri, C. M.; Arkharov, A. A.; Konstantinova, T. S.;
Kopatskaya, E. N.; Larionova, E. G.; Blinov, D.; Melnichuk, D.; Troitsky, I. (2009-03-01)...
- Arkharov, A. A.; Antoniucci, S.; Di Paola, A.; Konstantinova, T. S.;
Kopatskaya, E. N.; Li Causi, G.; Nisini, B. (May 2011). "Simultaneous monitoring...
- may have been
caused by
torque of its
accretion disk by the companion.
Kopatskaya, E. N.; Grinin, V. P.; Shakhovskoi, D. N.; Shulov, O. S. (April 2002)...
