National Science Olympiad Astronomy Event 2013 Stellar Evolution and Type II Supernovas Chandra X-Ray Education & Public Outreach Office Donna L Young, Lead Educator…
Where we are going? Wolf-Rayet Ring Nebulae Revisited I.Ciuca, Durham U., UK A.Marston, ESAC A.Pollock, ESAC Wolf-Rayet and their rings – a brief synopsis What are Wolf-Rayet…
Slide 120 April 2001AAO Workshop1 Optical & IR Interferometry Bill Tango School of Physics University of Sydney Slide 2 20 April 2001AAO Workshop2 Outline Historical…
Slide 1 .... Chepelare, Bulgaria, June 1-4, 2010 VII Bulgarian-Serbian Astronomical Conference ASTROINFORMATICS Astroinformatics for the Flare Stars in Stellar Clusters and…
Slide 1 WHERE IS FLUORINE? By: Ann Dyer, Samantha Sullivan, and Isaac Richter Slide 2 About Fluorine The most reactive element on the periodic table. Explodes with hydrogen.…
Slide 1 SLAC, October 7 th 2004 1 Multifrequency Strategies for the Identification of Gamma-Ray Sources Reshmi Mukherjee, Jules Halpern Marcus Ziegler Santa Cruz Institute…
Slide 1 Stellar Winds and Mass Loss Brian Baptista Slide 2 Summary Observations of mass loss Mass loss parameters for different types of stars Winds colliding with the ISM…
Slide 1 Goal: To understand the post main sequence evolutions of the most massive stars Objectives: 1)To learn about Eta Carinae and LBVs 2)To learn about what Wolf-Rayet…