Hostname: page-component-6bf8c574d5-w79xw Total loading time: 0 Render date: 2025-02-23T08:41:44.684Z Has data issue: false hasContentIssue false
  • English
  • Français

On the Bottom Magnetic Fields of Millisecond Pulsars

Published online by Cambridge University Press:  19 July 2016

Chengmin Zhang
Chengmin Zhang*
Affiliation:
School of Physics, The University of Sydney, NSW 2006, Australia

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 magnetic field strengths of most millisecond pulsars (MSPs) are about 108–9 gauss. The accretion-induced magnetic field evolution scenario here concludes that field decay is related to the accreted mass, that the minimum or bottom field stops at about 108 gauss for Eddington-limited accretion, and scales with the accretion rate as M1/2. The possibility of low field (∼ 107 gauss) MSPs has been proposed for future radio observations.

Type
Part 1: Neutron Star Formation and Evolution
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 47 - 48
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Cheng, K. S., & Zhang, C. M. 1998, A&A, 337, 441.Google Scholar
Romani, R. W. 1990, Nature, 347, 741.CrossRefGoogle Scholar
Shapiro, S. L., & Teukolsky, S. A. 1983, Black Holes, White Dwarfs and Neutron Stars, (New York: Wiley)CrossRefGoogle Scholar
Shibazaki, N., & Murakami, T., & Shaham, J., & Nomoto, K. 1989, Nature, 342, 656.CrossRefGoogle Scholar
van den Heuvel, E. P. J., & Bizaraki, O. 1995, A&A, 297, L41.Google Scholar
White, N., & Zhang, W. 1997, ApJ, 490, L87.CrossRefGoogle Scholar