This course relies entirely on class lectures by the instructor. The instructor will employ an interactive approach. The emphasis is on explaining processes to students and not on manipulating a bunch of symbols, aka equations. To achieve this goal, the instructor will explain the concept, solve one or two applications and then start solving problems and asking for input from the class at every point of the derivation. What the instructor writes on the board will be the result of the responses of the class. This interactive approach requires active class participation.

Temps présentiel : 30 heures

Charge de travail étudiant : 150 heures

Méthode(s) d'évaluation : Projets

Référence :
Osterbrock, D. E., & Ferland, G. J. 2005, Astrophysics of Gaseous Nebulae and Active Galaxies, University Science Book, ISBN 1891389343 Peterson, B. M. 2004, Introduction to Active Galactic Nuclei, Cambridge Univ. Press, ISBN 0521479118 Frank, J., King, A., & Raine, D. 1995, Accretion Power in Astrophysics, Cambridge Univ. Press 0521408636 Padmanabhan, T., Theoretical Astrophysics, Volume 3: Galaxies & Cosmology, Cambridge Univ. Press, Cambridge, 2002 Krolik, J. H. 1998, Active Galactic Nuclei, Princeton Univ. Press, ISBN 0691011516 Kembhavi, A., & Narlikar, J. V. 2006, Quasars and Active Galactic Nuclei, Cambridge Univ. Press, ISBN 0521479894