1 To Be or Not to Be: The Mysteries of Disk Formation Around Rapidly Spinning Be Stars Douglas R. Gies Department of Physics and Astronomy Center for High.
Thomas Henning and Dima Semenov Chemistry and Dynamics in Protoplanetary Disks Max-Planck-Institut für Astronomie, Heidelberg Courtesy of David E. Trilling.
Chapter 6: Planetological foundations for origins of life.
Global MHD Simulations of State Transitions and QPOs in Black Hole Accretion Flows
Chemical characterization of the first stages of protoplanetary disk formation Ugo Hincelin – 25 th June 2010 Collaborators :Valentine Wakelam (supervisor)