Hostname: page-component-77c89778f8-7drxs Total loading time: 0 Render date: 2024-07-19T07:24:14.373Z Has data issue: false hasContentIssue false
  • English
  • Français

Multiple Pulsar Ejection in Supernova Events∗

Published online by Cambridge University Press:  07 February 2017

F. Curtis Michel
F. Curtis Michel*
Affiliation:
Institute of Theoretical Astronomy, Cambridge, U.K.

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.

Fragmentation in the collapse of a supernova core, followed by energy loss in neutron star formation, is shown to lead to disruption of the resulting system. The elements of the system, some of which should be pulsars, can attain velocities of the order of 103 km/sec if currently quoted parameters are correct.

Type
Session 6
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 378 - 381
Copyright
Copyright © Reidel 1971 

References

Arnett, D.: 1967, Can. J. Phys. 45, 1621.CrossRefGoogle Scholar
Blaauw, A.: 1961, Bull. Astron. Inst. Neth. 15, 265.Google Scholar
Fowler, W. A. and Hoyle, F.: 1963, Nature 197, 533.CrossRefGoogle Scholar
Michel, F. C.: 1963, Astrophys. J. 138, 1097.CrossRefGoogle Scholar
Michel, F. C.: 1970, Astrophys. J. Letters 159, L25.CrossRefGoogle Scholar
Prentice, A. J. R.: 1970, Nature 225, 438.CrossRefGoogle Scholar
Richards, D. W., Pettengill, G. H., Counselman, C. C. III, and Rankin, J. M.: 1970, Astrophys. J. Letters 160, L1.CrossRefGoogle Scholar
Tsuruta, S. and Cameron, A. G. W.: 1966, Can. J. Phys. 44, 1895.CrossRefGoogle Scholar
Wheeler, J. A.: 1966, Ann. Rev. Astron. Astrophys. 4, 393.CrossRefGoogle Scholar