Everything you always wanted to know about stars… Material from Chapters 8 and 9 in Horizons by Seeds 0.
1 LHC Upgrades Albert De Roeck/CERN Implications of LHC results for TeV-scale physics: WG2 meeting 1/11/2011.
FNAL October 2003 SLHC prospects Albert De Roeck (CERN) 1 Physics Perspectives for a -Super LHC- Albert De Roeck CERN.
What do we use to measure distance to stars when parallax doesn’t work?
LENA Low Energy Neutrino Astrophysics F von Feilitzsch, L. Oberauer, W. Potzel Technische Universität München LENA Delta.
Ch9 THE SUN AND STARS The star we see by day. Ch9 The Sun, Our Star The Sun is an average star. From the Sun, we base our understanding of all stars in.
The Family of Stars Chapter 8:. Organizing the Family of Stars: The Hertzsprung-Russell Diagram We know: Stars have different temperatures, different.
July 20091 CMS experiment at LHC Geoff Hall Imperial College London Geoff Hall.
17.11.2014 3:13:51
Ratio of Three over Two Jet Cross Sections: Update 36 pb -1 P.Kokkas, I.Papadopoulos, C.Fountas University of Ioannina, Greece QCD High p T Meeting 17.
Properties of Stars
CMS experiment at LHC
