025_CompressibleFlows
Prof. dr. A. Achterberg, Astronomical Dept., IMAPP, Radboud Universiteit.
Baryonic Dark Matter and Galaxy Formation Françoise Combes, Observatoire de Paris 29 Avril 2005.
LOFAR & Particle acceleration in Galaxy Clusters Gianfranco Brunetti Institute of Radioastronomy –INAF, Bologna, ITALY.
HOT TIMES FOR COOLING FLOWS Mateusz Ruszkowski. Cooling flow cluster Non-cooling flow cluster gas radiates X-rays & loses pressure support against gravity.
Chandra Observations of Radio Sources in Clusters: Impact on the ICM and Tracers of High-z Systems Elizabeth Blanton University of Virginia Collaborators:
Psychology 023 Final Review. Final Exam Thursday April 15, 2004 2-5 pm AH Gym I am leaving for a weekend conference that evening so grades will not be.
1 Mirror Mode Storms in Solar Wind and ULF Waves in the Solar Wind C.T. Russell, L.K. Jian, X. Blanco-Cano and J.G. Luhmann 18 th STEREO Science Working.
LOFAR & Particle Acceleration: Radio Galaxies & Galaxy Clusters Gianfranco Brunetti Institute of Radioastronomy –INAF, Bologna, ITALY.
Elizabeth Blanton University of Virginia
Baryonic Dark Matter and Galaxy Formation
SEP “Campaign Events” for SHINE 2003
