I. Zalozhnykh
Moscow Engineering Physics Institute, Ural Federal University
Papers
2
Total Citations
48
H-Index
2
About
I. Zalozhnykh is a leading observational astrophysicist specializing in the study of explosive stellar transients and microquasars, with a particular focus on luminous red novae and black hole binary systems. Their most cited work, the 2017 discovery and analysis of MASTER OT J004207.99+405501.1 (M31LRN 2015), a rare luminous red nova in the Andromeda galaxy, has garnered 43 citations. This study provided critical insights into the hydrodynamics and evolution of these enigmatic stellar mergers, leveraging multicolour photometry from the MASTER Global Robotic Net telescopes. Zalozhnykh also made significant contributions to the monitoring of the 2015 superburst of V404 Cygni, a microquasar containing a black hole. Their 2019 paper, with 5 citations, presented 2,070 homogeneous photometric and polarization observations obtained from 16 robotic telescopes across eight global sites, offering an unprecedented dataset for understanding accretion and jet physics in black hole binaries. As a key member of the MASTER network, Zalozhnykh’s work exemplifies the power of robotic telescope arrays in capturing rare, time-critical astrophysical events, advancing our knowledge of stellar evolution and high-energy phenomena.
Research Focus
Key Achievements
Top Papers
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