Hostname: page-component-6bf8c574d5-vmclg Total loading time: 0 Render date: 2025-02-23T13:39:30.411Z Has data issue: false hasContentIssue false
  • English
  • Français

The Young Binary Pulsar J1740–3052

Published online by Cambridge University Press:  19 July 2016

I. H. Stairs
I. H. Stairs*
Affiliation:
Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada

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.

The young pulsar PSR J1740–3052, discovered in the Parkes Multibeam Pulsar Survey, is in a highly eccentric 8-month orbit with a companion of at least 11 solar masses. The up-to-date timing solution for this pulsar incorporates effects likely due to the spin mass quadrupole of the companion star; we discuss the implications for the geometry of the orbit. The pulsar signal displays increased dispersive delays as the pulsar passes behind its companion, indicating an interaction with the companion wind.

Type
Part 10: Radio Pulsar Timing
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 427 - 428
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Kaspi, V. M., Tauris, T., & Manchester, R. N. 1996a, ApJ, 459, 717.Google Scholar
Kaspi, V. M. et al. 1996b, Nature, 381, 584.CrossRefGoogle Scholar
Manchester, R. N. et al. 2001, MNRAS, 328, 17.CrossRefGoogle Scholar
Stairs, I. H. et al. 2001, MNRAS, 325, 979.CrossRefGoogle Scholar
Wex, N. 1998, MNRAS, 298, 997.Google Scholar