On the nature of pulsar radio emission
Authors:
- Maxim LyutikovMLMaxim Lyutikov
- Roger D. BlandfordRBRoger D. Blandford
- George MachabeliGMGeorge Machabeli
- 11 May 1999
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 305 (2) , 338-352
Abstract
No abstract availableKeywords
All Related Versions
This publication has 23 references indexed in Scilit:
- Size of the Vela Pulsar's Radio Emission Region: 500 KilometersThe Astrophysical Journal, 1997
- On the circular polarization in pulsar emissionMonthly Notices of the Royal Astronomical Society, 1991
- The Nature of Pulsar Subpulse DriftAustralian Journal of Physics, 1991
- Frequency dependence of the main pulse to interpulse separation for seven pulsarsThe Astrophysical Journal, 1986
- Wave propagation in pulsar magnetospheres - Dispersion relations and normal modes of plasmas in superstrong magnetic fieldsThe Astrophysical Journal, 1986
- Pair production in superstrong magnetic fieldsThe Astrophysical Journal, 1983
- Pair creation above pulsar polar caps - Geometrical structure and energetics of slot gapsThe Astrophysical Journal, 1983
- Pair creation above pulsar polar caps - Steady flow in the surface acceleration zone and polar CAP X-ray emissionThe Astrophysical Journal, 1981
- Acceleration of pulsars by asymmetric radiationThe Astrophysical Journal, 1975
- Amplification of Radiation by Relativistic Particles in a Strong Magnetic FieldMonthly Notices of the Royal Astronomical Society, 1975