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Petr Petrovich Petrov (b. 1945), a leading scientist at the Crimean Astrophysical Observatory, is widely known for his work on the variability of young stars having solar mass. He investigated magnetic and accretive activity in T Tauri stars and developed a concept for the magnetic activity of young stars.
Discovered on 22-10-1981 in Nauchnyj by Chernykh, N. S.