Spectroscopic Transits. The Rossiter-McClaughlin Effect 1 1 0 +v –v 2 3 4 2 3 4 The R-M effect occurs in eclipsing systems when the companion crosses.
Radiatively Driven Winds and Aspherical Mass Loss Stan Owocki U. of Delaware collaborators: Ken GayleyU. Iowa Nir Shaviv Hebrew U. Rich TownsendU. Delaware.
Breaching the Eddington Limit in the Most Massive, Most Luminous Stars Stan Owocki Bartol Research Institute University of Delaware Collaborators: Nir.
