Fermi rules out EC/CMB as the X-ray emission mechanism for 3C 273 Markos Georganopoulos 1,2 Eileen T. Meyer 3 1 University of Maryland, Baltimore County.
Magnetic dissipation in Poynting dominated outflows Yuri Lyubarsky Ben-Gurion University.
Mitch Begelman & Eric Coughlin JILA, University of Colorado ARE RELATIVISTIC JETS ALWAYS MAGNETIC?
Quasar large scale jets: Fast and powerful or weak and slow, but efficient accelerators? Markos Georganopoulos 1,2 1 University of Maryland, Baltimore.
Pulsar Wind Nebulae and Relativistic Shocks
Flow Vorticity and Rotation in Peripheral HIC Dujuan Wang 1 2014 CBCOS, Wuhan, 11/05/2014 University of Bergen, Norway.
Gamma-Ray-Bursts in Nuclear Astrophysics Giuseppe Pagliara Università di Ferrara Scuola di Fisica Nucleare “Raimondo Anni” Otranto 2006.
ARE RELATIVISTIC JETS ALWAYS MAGNETIC?
Flow Vorticity and Rotation in Peripheral HIC
Quasar large scale jets: Fast and powerful or weak and slow, but efficient accelerators?
