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Pulse Emission Mechanisms

  • Melrose D
Symposium - International Astronomical Union (2004) 218 349-356
DOI: 10.1017/s0074180900181367
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Abstract

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.

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APA

Melrose, D. (2004). Pulse Emission Mechanisms. Symposium - International Astronomical Union, 218, 349–356. https://doi.org/10.1017/s0074180900181367

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