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Whence the pulses?

Published online by Cambridge University Press:  12 April 2016

D.B. Melrose
D.B. Melrose*
Affiliation:
School of Physics, University of Sydney, NSW 2006, AUSTRALIA

Abstract

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Radio emission mechanisms for pulsars are reviewed with emphasis on five possible sites for the emission: the pair production front (PPF), two regions in the relativistically outflowing plasma (denoted ROP1 and ROP2) between the PPF and the light cylinder (LC), and two sited near the LC. Several maser emission mechanism are viable for ROP1, where radius-to-frequency mapping applies. Suggested Schott radiation from outside the LC is discussed critically.

Information

Type
Part 3 Radio Emission Processes
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 139 - 146
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Ardavan, H. 1992, in Hankins, Rankin and Gil (1992), p. 316 Google Scholar
Ardavan, H. 1994, MNRAS, 268, 361 Google Scholar
Arons, J. 1979, Space Sci.Rev., 24, 437 Google Scholar
Arons, J., Barnard, J.J. 1986, ApJ, 302, 120 Google Scholar
Backer, D.C. 1995, J.Astrophys.Astr., 16, 165 Google Scholar
Blandford, R.D. 1975, MNRAS, 170, 551 Google Scholar
Cordes, J.M. 1992, in Hankins, Rankin and Gil (1992), p. 253 Google Scholar
Cordes, J.M., Weisberg, J.M., Boriakoff, V. 1983, ApJ, 268, 370 Google Scholar
da Costa, A.A., Kahn, F.D. 1985, MNRAS, 215, 701 CrossRefGoogle Scholar
Daugherty, J.K., Harding, A.K. 1996, ApJ, 458, 278 CrossRefGoogle Scholar
Endean, G. 1995, MNRAS, 275, 309 Google Scholar
Ferguson, D.C. 1981, in Sieber and Wielebinski (1981), p. 141 Google Scholar
Grognard, R.J.-M. 1984, Solar Phys., 94, 165 Google Scholar
Hankins, T.H., Rankin, J.M., Gil, J.A. 1992, The Magnetospheric Structure and Emission Mechanisms of Radio Pulsars, Pedagogical University Press.Google Scholar
Lerche, I. 1970, ApJ, 162, 153 Google Scholar
Luo, Q., Melrose, D.B. 1992, MNRAS, 258, 616 Google Scholar
Luo, Q., Melrose, D.B. 1995, MNRAS, 276, 372 Google Scholar
Machabeli, G.Z., Usov, V.V. 1979, Sov.Astron.Lett., 5, 238 Google Scholar
Manchester, R.N., Taylor, J.H., Huguenin, G.R. 1975, ApJ, 196, 83 CrossRefGoogle Scholar
Melrose, D.B. 1978, ApJ, 225, 557 Google Scholar
Melrose, D.B. 1986, J.Geophys.Res., 291, 221 Google Scholar
Melrose, D.B. 1991, ARA&A, 29, 31 Google Scholar
Melrose, D.B. 1992a, in Hankins, Rankin and Gil (1992), p. 306 Google Scholar
Melrose, D.B. 1992b, Phil.Trans.Roy.Soc.London, A 341, 105 Google Scholar
Melrose, D.B. 1995, J.Astrophys.Astr., 16, 137 Google Scholar
Radhakrishnan, V. 1992, in Hankins, Rankin and Gil (1992), p. 367 Google Scholar
Rankin, J.M. 1983 ApJ, 274, 333 Google Scholar
Robinson, P.A. 1995, Phys.Plasmas, 2, 1466 Google Scholar
Robinson, P.A., Cairns, I.H., Gurnett, D.A. 1993 ApJ, 407, 790 Google Scholar
Rowe, E.T. 1992a&b, Aust.J.Phys., 45, 1&21 Google Scholar
Schott, G.A. 1912, Electromagnetic Radiation, Cambridge University Press Google Scholar
Sieber, W., Wielebinski, R. (eds) 1981, Pulsars, D. Reidel, Dordrecht Google Scholar
Stinebring, D.R., et al. 1984, ApJS, 55, 247 CrossRefGoogle Scholar
Thorsett, S.E. 1992, in Hankins, Rankin and Gil (1992), p. 143 Google Scholar
Ulmer, M.P. 1994, ApJS, 90, 789 Google Scholar
Wolszczan, A., Cordes, J.M. 1987, ApJ, 320, L35 Google Scholar
Xilouris, K.M., Kramer, M., Jessner, A., Wielebinski, R. 1994, A&A, 288, L17 Google Scholar
Yadigaroglu, L.-A., Romani, R.W. 1995, ApJ, 449, 211 Google Scholar