Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-30T10:34:59.950Z Has data issue: false hasContentIssue false
  • English
  • Français

Geometrical effects on radio pulsar profiles and spectra

Published online by Cambridge University Press:  12 April 2016

Wolfgang Sieber
Wolfgang Sieber*
Affiliation:
Fachhochschule Niederrhein, PF 2850, D-4 7728 Krefeld, Germany

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Considering the geometry of the hollow-cone model of radio pulsar emission in detail, one is led to the conclusion that several well-known observed effects may be explained quite easily purely on geometrical terms. It is shown that a steepening of the spectrum (cut-off) may be expected for certain geometrical situations as well as variations in component spectra, e.g. steeper spectra for the central component. These effects appear in addition to the already existing physical variations with frequency.

Type
Part 3 Radio Emission Processes
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 167 - 170
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Kramer, M., Wielebinski, R., Jessner, A., Gil, J.A., Seiradakis, J.H. 1994, A&AS, 107, 515 Google Scholar
Phillips, J.A., Wolszczan, A. 1992, ApJ, 385, 273 Google Scholar
Radhakrishnan, V., Cooke, D.J. 1969, Astrophys. Lett., 3, 225 Google Scholar
Ruderman, M.A., Sutherland, P.G. 1975, ApJ, 196, 51 Google Scholar
Sieber, W. 1973, A&A, 28, 237 Google Scholar
Sieber, W. 1996, A&A, in pressGoogle Scholar
Sieber, W., Reinecke, R., Wielebinski, R. 1975, A&A, 38, 169 Google Scholar
Thorsett, S.E. 1991, ApJ, 377, 263 Google Scholar