Galactic pulsar population and the origin of high-energy cosmic rays
- 18 April 2002
- journal article
- Published by IOP Publishing in Journal of Physics G: Nuclear and Particle Physics
- Vol. 28 (6) , 1275-1286
- https://doi.org/10.1088/0954-3899/28/6/310
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- Ultra–High-Energy Cosmic Rays from Young Neutron Star WindsThe Astrophysical Journal, 2000
- Origin of the highest energy cosmic rays and the Galactic haloNuclear Physics A, 2000
- Why are supernovae in our Galaxy so frequent?Monthly Notices of the Royal Astronomical Society, 1999
- Cosmic ray anisotropies at very high energies expected for new models of the Galactic magnetic fieldJournal of Physics G: Nuclear and Particle Physics, 1994
- Magnetically striped relativistic magnetohydrodynamic winds - The Crab Nebula revisitedThe Astrophysical Journal, 1990
- Energetic Radiation from Rapidly Spinning Pulsars. II. VELA and CrabThe Astrophysical Journal, 1986
- Energetic radiation from rapidly spinning pulsars. I - Outer magnetosphere gaps. II - VELA and CrabThe Astrophysical Journal, 1986
- Current flow in pulsar magnetospheresThe Astrophysical Journal, 1976
- On the Nature of Pulsars. III. Analysis of ObservationsThe Astrophysical Journal, 1970
- Pulsar ElectrodynamicsThe Astrophysical Journal, 1969