Hostname: page-component-8448b6f56d-mp689 Total loading time: 0 Render date: 2024-04-19T05:44:49.504Z Has data issue: false hasContentIssue false
  • English
  • Français

Crab-Like Supernova Remnants

Published online by Cambridge University Press:  04 August 2017

R.H. Becker
R.H. Becker*
Affiliation:
Physics Department, University of California, Davis, CA 95616 Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory

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.

Crab-like SNR are markers for recently formed pulsars. The current catalog of 15 objects allows a direct measure of the space distribution of pulsars, the beaming factor of pulsars, and the energetics at young pulsars. The 15 Crab-like SNR are equally divided between those with surroundings shells and those without. No other properties appear to correlate with the presence or lack of a shell. The ratio of 10 to 1 between all remnants and Crab-like remnants has important implications for the formation of pulsars.

Type
I. Rotation-Powered Pulsars
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 91 - 97
Copyright
Copyright © Reidel 1987 

References

Becker, R.H. 1983 in Supernova Remnants and Their X-ray Emission (ed. by Danziger, and Gorenstein, ) D. Reidel, Dordrecht, p. 329.Google Scholar
Becker, R.H. and Helfand, J. 1984 Ap. J. 281, 650.Google Scholar
Becker, R.H. and Helfand, J. 1985 Ap. J. (Letters) 297, L25.Google Scholar
Becker, R.H. and Helfand, J. 1986 in preparation.Google Scholar
Caswell, et al. 1980, MNRAS 190, 882.Google Scholar
Davelaar, et al. 1986 Ap. J. (Letters) 300, L59.CrossRefGoogle Scholar
Downes, et al. 1986 MNRAS 218, 393.CrossRefGoogle Scholar
Green, 1986 MNRAS 218, 533.Google Scholar
Harnden, et al. 1985 Ap. J. 299, 828.Google Scholar
Helfand, D.J. 1984, Adv. Space Res. 3, 29.Google Scholar
Helfand, D.J. and Becker, R.H. 1986 Ap. J., in press.Google Scholar
Hughes, et al. 1984, Ap. J. 283, 147.Google Scholar
Kriss, G. et al. 1985 Ap. J. 288, 703.Google Scholar
Milne, D. et al. 1985 Proc. Astron. Soc. Aust. 6, 78.CrossRefGoogle Scholar
Minkowski, R. 1971 in The Crab Nebula (ed. by Davies, and Smith, ) D. Reidel, Dordrecht, p. 241.CrossRefGoogle Scholar
Reich, et al. 1985 Astron. Astrophys. 151, L10.Google Scholar
Reich, et al. 1984 Astron. Astrophys. 133, L4.Google Scholar
Reynolds, S.P. and Aller, H. 1985 A.J. 90, 2312.CrossRefGoogle Scholar
Seward, F. et al. 1984 Ap. J. 281, 650.Google Scholar
Strom, R. and Blair, W. 1985 Astron. Astrophys. 149, 254.Google Scholar
Tuohy, , et al. 1983 Ap. J. 268, 778.Google Scholar
Velusamy, T. 1985 in The Crab Nebula and Related Supernova Remnants (ed. by Kafatos, and Henry, ) Cambridge Univ. Press, p. 115.Google Scholar
Weiler, K.W. 1983 in Supernova Remnants and Their X-Ray Emission (ed. by Danziger, and Gorenstein, ) D. Reidel, Dordrecht, p. 299.CrossRefGoogle Scholar
Wilson, A. 1980 Ap. J. (Letters) 241, L19.Google Scholar
Wilson, A. 1986 Ap. J. Google Scholar