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Michael De Robertis is a Professor Emeritus at York University’s Faculty of Science. His research primarily focuses on Active Galactic Nuclei (AGN), particularly Seyfert galaxies, which are known for their remarkable nuclear activities. He is interested in understanding the origins of nuclear activity in these galaxies, emphasizing their intense emissions resulting from accretion processes involving gas and stars around supermassive black holes. In addition, he explores the role of the environments around Seyfert galaxies in influencing their activities. Apart from AGNs, he also studies cool dwarf stars and the structural components of the Milky Way galaxy. De Robertis’ investigation into the majority of stars in our solar neighborhood, primarily late-type (M) dwarfs and subdwarfs, highlights the kinematics of these stars along with their surface temperatures and metal abundances through imaging techniques. His work includes both computational and experimental research methodologies in astronomy and astrophysics, making significant contributions to our understanding of galactic structure.
Department of Liberal Arts & Professional Studies graduate programs generally follow the Faculty of Graduate Studies (FGS) B+ minimum requirement.