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Pulse Emission Mechanisms

Published online by Cambridge University Press:  19 July 2016

Don Melrose*
Affiliation:
School of Physics, University of Sydney, NSW 2006, Australia

Abstract

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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.

Type
Part 8: Pulsar Electrodynamics and Emission Theory
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Arendt, P. N. Jr, & Eilek, J. A. 2002, ApJ, 581, 451.Google Scholar
Blandford, R. D. 1975, MNRAS, 170, 551.Google Scholar
Bougeret, J.-L., & Steinberg, J.-L. 1977, A&A, 61, 777.Google Scholar
Canuto, V., Lodenquai, J., & Ruderman, M. 1971, Phys. Rev. D, 3, 2303.Google Scholar
Cheng, K. S., Ho, C., & Ruderman, M. A. 1986, ApJ, 300, 522.Google Scholar
Cheng, K. S., & Zhang, L. 1999 ApJ, 515, 337.Google Scholar
Daugherty, J. K., & Harding, A. K. 1989 ApJ, 336, 871.Google Scholar
Dermer, C. D. 1990, ApJ, 360, 214.Google Scholar
Duncan, R. A. 1979, Solar Phys., 63, 389.Google Scholar
Gangadhara, R. T. & Gupta, Y. 2001, ApJ, 555, 31.Google Scholar
Gedalin, M., Gruman, E., & Melrose, D. B. 2002, MNRAS, 337, 422.Google Scholar
Herold, H. 1979 Phys. Rev. D, 19, 2868.Google Scholar
Hibschman, J. A., & Arons, J. 2001, ApJ, 560, 671.Google Scholar
Hirotani, K., & Shibata, S. 2001, MNRAS, 325, 1228.Google Scholar
Kazbegi, A. Z., Machabeli, G. Z., & Melikidze, G. I. 1991, MNRAS, 263, 377.Google Scholar
Kirk, J. G., Skæraasen, O., & Gallant, Y. 2002, A&A, 388, L29.Google Scholar
Luo, Q., & Melrose, D. B. 1992, MNRAS, 258, 616.Google Scholar
Luo, Q., & Melrose, D. B. 1995, MNRAS, 276, 631.Google Scholar
Lyutikov, M., Blandford, R. D., & Machabeli, G. 1999, MNRAS, 305, 338.Google Scholar
Machabeli, G. Z., & Usov, V. V. 1979, Sov. Astron. Lett., 5, 445.Google Scholar
McKinnon, M. M., & Stinebring, D.R. 2000, ApJ, 529, 435.CrossRefGoogle Scholar
Melrose, D. B. 1975, Solar Phys., 43, 79.Google Scholar
Melrose, D. B. 1978, ApJ, 225, 557.Google Scholar
Melrose, D. B., & Gedalin, M. 1999, ApJ, 521, 351.Google Scholar
Melrose, D. B., & Sy, W. 1972, Ap&SS, 17, 343.Google Scholar
Radhakrishnan, V., & Deshpande, A.A. 2001, A&A, 379, 551.Google Scholar
Romani, R. 1996, ApJ, 470, 469.Google Scholar
Rowe, E. T. 1995, A&A, 296, 275.Google Scholar
Usov, V. V. 1987, ApJ, 320, 333.Google Scholar
Usov, V. V., & Melrose, D. B. 1996, ApJ, 464, 306.Google Scholar
Weise, J. I., & Melrose, D. B. 2002, MNRAS, 329, 115.Google Scholar
Zhang, B., & Harding, A. K. 2000, ApJ, 532, 1150.Google Scholar