Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-26T03:15:53.213Z Has data issue: false hasContentIssue false
  • English
  • Français

On the timing histories of the crab, PSR1509-58 and PSR0540-69

Published online by Cambridge University Press:  12 April 2016

Alberto Carramiñana  and
César Alvarez
Alberto Carramiñana
Affiliation:
Instituto Nacional de Astrofísica, Optica y Electrónica Apartado Postal 51 y 216, Puebla 72000, Pue., MEXICO
César Alvarez
Affiliation:
Instituto Nacional de Astrofísica, Optica y Electrónica Apartado Postal 51 y 216, Puebla 72000, Pue., MEXICO

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.

A simple model of a combined magnetic dipole, gravitational and/or magnetic quadrupole and particle accelerator is applied to simulate the time behaviour of the timing parameters of PSR 0531+21, PSR 1509-58 and PSR0540-69, as well as their energy budget. The model restricts the allowed values for the second braking index and is therefore testable through measurements of .

Type
Part 2 Precision Measurements
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 107 - 108
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Dermer, C.D. & Sturner, S.J., 1994 ApJ, 420, L75 Google Scholar
Gouiffes, C., Finley, J.P. & Ögelman, H. 1992 ApJ, 394, 581 Google Scholar
Kaspi, V.M. et al. 1994, ApJ, 422, L83.Google Scholar
Ostriker, J.P. & Gunn, J.E. 1969, ApJ, 157, 1395 Google Scholar
Pacini, F. 1968, Nat, 219, 145 Google Scholar