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Pierre Bergeron is an Associate Professor in the Department of Physics at the Université de Montréal. He specializes in the study of white dwarf stars, focusing on the calculation of model atmospheres. His research interests include the evolution and characteristics of white dwarfs, which are the final evolutionary stage for more than 97% of stars in the galaxy. He employs spectroscopic methods to measure fundamental parameters such as surface temperature and chemical composition of these compact objects. His work is pivotal in understanding stellar remnants and also encompasses the pulsating white dwarfs known as ZZ Ceti stars. Additionally, Bergeron is involved in numerous research projects and collaborations that leverage contemporary observatories and resources to enhance the empirical data available for his studies. Throughout his career, he has received several awards for teaching excellence and has contributed significantly to academic education and supervision of graduate students in astrophysics.
Université de Montréal • Montreal, QC
Teaching and researching in astrophysics, particularly the study of white dwarf stars.
Most programs require French B2 level; specific departments may require C1 or C2.