Hostname: page-component-8448b6f56d-mp689 Total loading time: 0 Render date: 2024-04-16T12:01:33.964Z Has data issue: false hasContentIssue false
  • English
  • Français

An Arithmetic Method for Mean Pulse Profile De-disperse of pulsars

Published online by Cambridge University Press:  12 April 2016

X.J. Wu  and
X.F. Liu
X.J. Wu
Affiliation:
Beijing Astrophysics Center, CAS-PKU, Beijing 100871, China Astronomy Department, Peking University, Beijing 100871, China
X.F. Liu
Affiliation:
Beijing Astrophysics Center, CAS-PKU, Beijing 100871, China Astronomy Department, Peking University, Beijing 100871, China

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.

In this paper we discuss an arithmetic method for mean pulse profile de-disperse. We proceed from the principle of dispersion measure, and invert the de-dispersion problem as to refutations of solving integral equations. Under idealization condition, the refutations results fit very well with the given theoretical curvature.

Type
Part 3. Studies of Radio Emission
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 285 - 286
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Kuzmin, A.D., & Izvekova, V.A., MNRAS, 1993, 260, 724 CrossRefGoogle Scholar
Kramer, M., 1994, A&AS, 107, 527 Google Scholar
Wu, X.J. & Manchester, R.N., Science of China, 1993, 136, 468 Google Scholar
Wu, X.J., Xu, W. & Rankin, J.M., Proc. IAU colloq., 128, ed. Hankin, , Rankin, & Gil, , 1992, 172 Google Scholar
Wu, X.J., Gao, X.Y., Rankin, J.M., Xu, W. & Malofeev, V.M., 1998 AJ. 116, 1984 Google Scholar