Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-25T15:40:07.478Z Has data issue: false hasContentIssue false
  • English
  • Français

Orbital Trends of Binary Pulsars

Published online by Cambridge University Press:  19 July 2016

Tapan Chatterjee
Tapan Chatterjee*
Affiliation:
University of Puebla (FCC), Apartado Postal 1316, Puebla, 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.

We try to understand the eccentricity of high-mass binary pulsars using some methods of statistical mechanics.

Type
Part 1: Neutron Star Formation and Evolution
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 53 - 54
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Lynden-Bell, D., & Pringle, J. E. 1974, MNRAS, 168, 603.Google Scholar
Magalinsky, V. B., & Chatterjee, T. K. 2000, Astron. Astrophys. Trans., 18, 807.Google Scholar
Thorsett, S. E., Arzoumanian, Z., McKinnon, M. M., & Taylor, J. H. 1993, ApJ, 405, L29.Google Scholar
Verbunt, F. 1990, in Neutron Stars and their Birth Events, ed. Kundt, W., (Dordrecht: Kluwer), p. 179.Google Scholar
Wolszczan, A., 1991, Nature, 350, 688.Google Scholar