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Pulsar radio emission beams

Published online by Cambridge University Press:  12 April 2016

Jaroslaw Kijak
Jaroslaw Kijak*
Affiliation:
J, Kepler Astronomical Center, Pedagogical University, Lubuska 2, PL-65-265 Zielona Góra, Poland

Abstract

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We study the structure of the pulsar beam using the analysis of beam radius. We indentify three emission cones in radio beams. The dependence of the beam radius on frequency is obtained.

Type
Part 3. Studies of Radio Emission
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 195 - 196
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Gil, J., Gronkowski, P., & Rudnicki, W. 1984, A&A, 132, 312 Google Scholar
Gil, J., Krawczyk, A., 1997, A&A, 280, 143 Google Scholar
Kijak, J. Gil, J. 1998, MNRAS, 299, 855 Google Scholar
Kijak, J., Kramer, M., Wielebinski, R., & Jessner, A. 1998, A&A, 127, 153 Google Scholar
Manchester, R.N., Han, J.L., & Qiao, J. 1998, MNRAS, 295, 280 Google Scholar
Mitra, D. & Deshpande, A.A., 1999, A&A, 346, 906 Google Scholar
Ommen, T.D., D’Alessandro, F., Hamilton, P.A., & McCulloch, P.M. 1997, 287, 307 Google Scholar