Sakdawoot Maungkorn

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About

Sakdawoot Maungkorn is an observational astronomer specializing in the photometric analysis of variable stars, particularly eclipsing binary systems. His research focuses on deriving precise orbital parameters and physical properties of these stellar pairs through light curve modeling, contributing to our understanding of stellar evolution and binary star dynamics. Maungkorn’s most cited work, “A photometric analysis of the neglected EW-type binary V336 TrA” (2017), has garnered 11 citations, highlighting its significance in characterizing a previously understudied W Ursae Majoris-type contact binary. This study provided key measurements of the system’s mass ratio, inclination, and fill-out factor, offering insights into the evolutionary status of such close binaries. Maungkorn’s contributions are particularly valuable for filling gaps in the catalog of variable stars, enabling more comprehensive statistical studies of binary star populations. His meticulous photometric approach and dedication to analyzing overlooked systems underscore his role in advancing stellar astrophysics, making his work a foundation for future research on contact binaries and their role in galactic stellar evolution.