K. V. Sokolovsky

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About

K. V. Sokolovsky is a distinguished astrophysicist specializing in time-domain astronomy, cataclysmic variable stars, and transient phenomena. His research focuses on the discovery and characterization of exotic binary systems, particularly AM CVn-type ultracompact binaries—rare, helium-rich systems that offer critical insights into stellar evolution and gravitational wave sources. Sokolovsky’s major contribution includes the identification and analysis of TCP J07222683+6220548, a new AM CVn system exhibiting infrequent, dramatic outbursts with a magnitude change of ΔV = 7.6. This work, published in 2025 and already garnering 2 citations, showcases his skill in leveraging wide-field surveys like the New Milky Way survey and ASAS-SN to detect rare transients. His findings deepen our understanding of binary mass transfer and accretion physics. Beyond this, Sokolovsky is recognized for his expertise in optical and infrared monitoring of variable stars, contributing to large-scale transient follow-up networks. With a career marked by meticulous observational work and rapid-response discoveries, he continues to shape the study of compact binaries and their explosive behavior, making him a key figure in modern time-domain astrophysics.