The origin of stars is an issue not only of great intrinsic interest, but also key to understanding galaxy and planet formation. We will delve into the physics of this process, from the condensation of diffuse, interstellar matter to the ignition of hydrogen fusion. We will also study star formation on galactic scales. Finally, we will see how the disks created around individual stars create orbiting planets. This course is open to graduate students in Astronomy, Physics, and Earth and Planetary Sciences. There are no formal prerequisites.
Office: 423 Campbell
Phone: 642-1164
Office hours: 1-2 pm, Tues, Thurs or anytime by appointment
The Formation of Stars, Stahler & Palla (2004, Wiley)
Tues/Thurs, 10:30 am - noon, 501 Campbell Hall
06182