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Studying Pulsar Emission Regions Using Interstellar Scattering

Published online by Cambridge University Press:  12 April 2016

Carl R. Gwinn
Carl R. Gwinn*
Affiliation:
University of California, Santa Barbara

Abstract

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Radio-wave scattering in the interstellar plasma provides the means to circumvent the diffraction limit for earth-based instruments, and to image the emission regions of pulsars. For the past 25 years, observers have sought to exploit this fact to learn how pulsars shine. I review the techniques developed, and summarize measurements of size of emission regions of pulsars to date.

Type
Chapter Two Pulsars: Their Scattering and Intrinsic Properties
Information
International Astronomical Union Colloquium , Volume 182: Sources and Scintillations: Refraction and Scattering in Radio Astronomy , 2001 , pp. 65 - 70
Copyright
Copyright © Kluwer 2001

References

Cordes, J.M., Weisberg, J.M. and Boriakoff, V.: 1983, Astrophys. J. 268, 370.Google Scholar
Desai, K.M., Gwinn, C.R., Reynolds, J.R., King, E.A., Jauncey, D., Flanagan, C, Nicolson, G., Preston, R.A. and Jones, D.L.: 1992, Astrophys. J. 393, L75.Google Scholar
Gupta, Y., Bhat, N.D.R. and Rao, A.P.: 1999, Astrophys. J. 520, 173.CrossRefGoogle Scholar
Gwinn, C.R., Britton, M.C., Reynolds, J.R., Jauncey, D.L., King, E.A., McCulloch, P.M., Lovell, J.E.J., Flanagan, C.S. and Preston, R.A.: 1998, Astrophys. J. 505, 928.Google Scholar
Gwinn, C.R., Britton, M.C., Reynolds, J.E., Jauncey, D.L., King, E.A., McCulloch, P.M., Lovell, J.E.J., Flanagan, C.S. and Preston, R.A.: 2000, Astrophys. J. 531, 902.Google Scholar
Gwinn, C.R., Ojeda, M.J., Britton, M.C., Reynolds, J.R., Jauncey, D.L., King, E.A., McCulloch, P.M., Lovell, J.E.J., Flanagan, C.S., Smits, D.P., Preston, R.A. and Jones, D.L.: 1997, Astrophys. J. 483, 53.Google Scholar
Macquart, J.-P., Johnston, S., Walker, M. and Stinebring, D.: 2000, in: Kramer, M., Wcx, N. and Wielebinski, N. (eds.), Pulsar Astronomy - 2000 and Beyond, Astronomical Society of the Pacific, p. 215.Google Scholar
Phillips, J.A.: 1992, Astrophys. J. 385, 282.CrossRefGoogle Scholar
Roberts, J.A. and Ables, J.G.: 1982, Mon. Not. R. Astron. Soc. 201, 1119.Google Scholar
Smirnova, T.V., Shishov, V.I., and Malofeev, V.M.: 1996, Astrophys. J. 462, 289.CrossRefGoogle Scholar
Wolszczan, A., Bartlett, J.E. and Cordes, J.M.: 1988, in: Cordes, J.M., Rickett, B.J. and Backer, D.C. (eds.), Radio Wave Scattering in the Interstellar Medium, American Institute of Physics, p. 145.Google Scholar
Wolszczan, A. and Cordes, J.M.: 1987, Astrophys. J. 320, L35.CrossRefGoogle Scholar