Understanding circumstellar disks requires a broad range of scientific knowledge, including chemical processes, the properties of dust and gases, hydrodynamics and magnetohydrodynamics, radiation transfer, and stellar evolution—all of which are covered in this course, which will be indispensable for graduate students, seasoned researchers, or even advanced undergrads setting out on the study of planetary evolution.

Temps présentiel : 30 heures

Charge de travail étudiant : 150 heures

Méthode(s) d'évaluation : Projets

Référence :
Physical Processes in Circumstellar Disks around Young Stars, Edited by PAULO J. V. GARCIA Physics and Chemistry of Circumstellar Dust Shells, Hans-Peter Gail, Erwin Sedlmayr