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About

I. Myserlis is an astrophysicist specializing in the magnetic field structures of molecular clouds and the role of polarization in tracing star formation processes. His work focuses on the poorly understood early stages of stellar birth, particularly within quiescent clouds like the Polaris Flare. His most-cited paper, "Optical polarization map of the Polaris Flare with RoboPol" (2015, 47 citations), presents the first detailed map of the plane-of-the-sky magnetic field orientation in this region, using polarized starlight as a tracer. This contribution provides critical insights into how magnetic fields influence cloud dynamics and the initial conditions for star formation. Myserlis’s research is notable for advancing observational techniques in polarimetry and for shedding light on the magnetic environments of quiescent clouds, which are key to understanding the earliest stages of stellar evolution. His work continues to inform models of cloud collapse and star formation.