2003/08/27 by Don Melrose, Melrose, Don
Engineering · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Geophysics and Sensor Technology #Pulsars and Gravitational Waves Research #Superconducting Materials and Applications #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0308471
To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler
arxiv created 2003/08/27 · openalex publication_date 2003/08/27 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
High-energy and radio emission mechanisms for pulsars are reviewed. The source region for high energy emission remains uncertain. Two preferred radio emission mechanism are identified. Some difficulties may be resolved by appealing to nonstationary pair creation distributed widely in height.