Bio

My research interests focus on neutral hydrogen (H I) in galaxies, particularly its role in shaping the morphology, structure, and classification of galaxies. I am interested in studying the spatial distribution and kinematics of H I gas to understand how it influences galaxy evolution, interaction dynamics, and large-scale morphological features such as spiral arms, warps, tidal tails, and disks. I am also interested in the development and application of morphological classification techniques, including both traditional visual classification and modern machine learning or quantitative methods.