Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-05T03:26:40.396Z Has data issue: false hasContentIssue false
  • English
  • Français

The Birthplaces of Pulsars

Published online by Cambridge University Press:  14 August 2015

A. G. Lyne
A. G. Lyne*
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Cheshire, United Kingdom

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.

With the refinement of the estimates of electron density in the Galaxy it is clear that pulsars have z distances away from the galactic plane of a few hundred parsec. There is now a very strong indication that young pulsars lie at small z distances, suggesting that pulsars originate in a small z population and are given velocities of about 100 km s-1 at birth.

Type
Part 3: Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 369 - 372
Copyright
Copyright © Reidel 1974 

References

Downs, G. S. and Reichley, P. E.: 1971, Astrophys. J. Letters 163, L11.CrossRefGoogle Scholar
Ewing, M. S., Batchelor, R. A., Friefield, R. D., Price, R. M., and Staelin, D. H.: 1970, Astrophys. J. Letters 162, L169.Google Scholar
Galt, J. A. and Lyne, A. G.: 1972, Monthly Notices Roy. Astron. Soc. 158, 281.Google Scholar
Gold, T. and Newman, H. M.: 1970, Nature 227, 151.CrossRefGoogle Scholar
Gunn, J. E. and Ostriker, J. P.: 1970, Astrophys. J. 160, 979.CrossRefGoogle Scholar
Lang, K. R. and Rickett, B. J.: 1970, Nature 225, 528.CrossRefGoogle Scholar
Oort, J. H.: 1965, Stars and Stellar Systems 5, 455.Google Scholar
Poveda, A. and Woltjer, L.: 1968, Astron. J. 73, 65.Google Scholar
Prentice, A. J. R.: 1970, Nature 225, 438.CrossRefGoogle Scholar
Rickett, B. J.: 1970, Monthly Notices Roy. Astron. Soc. 150, 67.Google Scholar