Slide 1Accretion Processes in Star Formation Lee Hartmann Cambridge Astrophysics Series, 32 Cambridge University Press (also from Nuria Calvet talks (2004) (continued) Slide…

Slide 1 NJIT Physics 320: Astronomy and Astrophysics – Lecture X Carsten Denker Physics Department Center for Solar–Terrestrial Research Slide 2 November 5th, 2003NJIT…

Slide 1 Inflating Fat Bubbles in Clusters of Galaxies by Slow Wide Jets Assaf Sternberg (did the work) Noam Soker (speaker today) Technion, Israel July 2008 Slide 2 Goal:…

Slide 1 Induced Star Formation in the Orion and Monoceros Molecular Clouds Hsu-Tai Lee and Wen-Ping Chen National Central University, Institute of Astronomy Slide 2 Outline…

Additional Image Set for 2007 Science Olympiad http://eezway.org/clinic/Astronomy/Addnl_Card_set.pdf 35. DEM L316: Supernova Remnants Deconstructed This composite X-ray (red…

Warm up The sun is 4.6 billion years old â how can it continue to produce so much heat and light? Nuclear reactions Create new atoms â different elements Fission â splitting…

Light element abundances in NGC 5128 from planetary nebulae Jeremy R. Walsh, ESO George H. Jacoby, WIYN Reynier Pelletier, Kapteyn Lab., Groningen Nic A. Walton, IoA, Cambridge…

Warm up The sun is 4.6 billion years old â how can it continue to produce so much heat and light? Nuclear reactions Create new atoms â different elements Fission â splitting…

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…

Chapter 10: The Death of Stars (part b) The evolution of low-mass vs. that of high-mass stars. Planetary nebulae and the formation of white dwarf stars. Supernova explosions:…