Acceleration by pulsar winds in binary systems
Alice K. Harding, Thomas K. Gaisser, Laboratory for High Energy Astrophysics (Goddard Space Flight Center)
Laboratory for High Energy Astrophysics, National Aeronautics and Space Administration, Goddard Space Flight Center, 1990 - Pulsars - 31 pages
7 pages matching field from Eqn in this book
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accelerated particles accelerated protons accretion flow Alfven radius Ballmoos binary pulsars binary system companion mass companion radius companion star atmosphere companion star wind confinement Crab nebula Cyg X-3 system Cygnus X-3 density dependence determined diffusion dipole luminosity Eddington limit Eichler electron factor field from Eqn Figure Gaisser gamma-ray induced wind interaction interstellar medium Kennel and Coroniti labeled with values magnetic field magnetosphere mass loss rate maximum energy maximum proton acceleration maximum proton energy Mmax neutron star observed orbital period pair production parameter particle acceleration particle energy predicted flux pressure balance Protheroe proton acceleration energy pulsar light cylinder pulsar spin-down pulsar wind power pulsar wind shock radiation pressure radio pulsar require Ruderman scale height Shaham shock acceleration shock location shock radius solid angle spectrum stellar wind Table Tavani thermal wind model upper limit VHE and UHE wind or atmosphere wind ram pressure wind terminal velocity X-ray