Table of ContentsThe Rocket Science of Launching Stellar Disks Where do stars, planets, we, come from?? Summary: Disks from Infalling Matter The Rocket Science of Launching Stellar Disks Spectral lines & Doppler shift Rotational Broadening of Photospheric Absorption Lines Formation of a P-Cygni Line- Profile Hydrodynamical Simulations of Wind Compressed Disks WCD Inhibition by Non-Radial Forces WCD Inhibition by Poleward Line-Force Line-Profile Variations from Non-Radial Pulsation First try: Localized Equatorial Bright Spots Rotational Modulation of Hot-Star Winds Symmetric Bright Spot on Rapidly Rotating Be Star RDOME Radiatively Driven Orbital Mass Ejection Time Evolution of Single Prograde Spot Outward Viscous Diffusion of Ejected Gas |
Author: Stan Owocki
Email: owocki@bartol.udel.edu Home Page: www.bartol.udel.edu/~owocki Other information: |