Star formation and Feedback at z>1 Alice Shapley (UCLA) Collaborators: (UCLA) Daniel Nestor, Robin Mostardi, Kathy Kornei, Kristin Kulas, Kevin Hainline, David Law, Sarah…

Problem 9.9 Center for Solar-Terrestrial Research Problem 9.12 At wavelength where the opacity is greatest, the value of s is smallest. If the temperature of the star’s…

THE PLUS-MINUS METHOD OF INTERPRETING SEISMIC REFRACTION SECTIONS * # J. G. HAGE&30RX ** ABSTRACT The elastic impulse from an explosion is propagated through the earth…

Inflating Fat Bubbles in Clusters of Galaxies by Slow Wide Jets Assaf Sternberg (did the work) Noam Soker (speaker today) Technion, Israel July 2008 Goal: To form âFatâ…

Conclusions The prototype z Pup (O4 I) has X-ray emission line profiles consistent with a simple spherically symmetric wind shock model. What can lead to lines that are broad,…

Conclusions The prototype z Pup (O4 I) has X-ray emission line profiles consistent with a simple spherically symmetric wind shock model. What can lead to lines that are broad,…