Abstract
Observations of a new type of rapidly varying radio source have recently been reported1. The principal characteristics of the four sources so far discovered may be summarized as follows—sharp pulses of radiation are received, separated by comparatively long intervals which themselves are remarkably constant (with variations of ≲ 1 part in 2 × 107 during the past 3 or 4 months). The pulse duration is no more than ~ 0·016 s, while the period is 1#x00B7;3372795 ±0#x00B7;0000020 s (ref. 1). We understand that the other objects show similar sharp pulses at intervals of the order of 1 s, which, although not identical, strongly suggest that a new type of physical system has been discovered. Hewish et al. propose that the objects may be pulsating white dwarfs or neutron stars. Although this may prove to be correct, there are certain difficulties associated with the constancy of the observed period. We suggest an alternative explanation for the observed phenomena.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., and Collins, R. A., Nature, 217, 709 (1968), (Paper 1); and Hewish, A., Cavendish Colloquium, 20 February, 1968.
Liebes, Jun., S., Phys. Rev., 113 B, 835 (1963).
Meltzer, D., and Thome, K. S., Ap. J., 145, 514 (1966).
Hoyle, F., and Narlikar, J. V., Proc. Roy. Soc., 218, 465 (1963).
Allen, C. W., Astrophysical Quantities, second ed., 238 (Athlone Press, London, 1963).
Jeans, J., Astronomy and Cosmogony, second ed. (Dover Publ., 1961).
Lyttleton, R. A., The Stability of Rotating Liquid Masses (Cambridge Univ. Press, 1953).
Hoyle, F., Narlikar, J. V., and Wheeler, J. A., Nature, 203, 914 (1964).
Landau, L. D., and Lifshitz, E. M., Classical Theory of Fields (Addison Wesley, 1951).
Zee, A., and Wheeler, J. A., as in Ann. Rev. Astro. Astrophys., 4, 393 (1966).
Tsuruta, S., and Cameron, A. G. W., Nature, 211, 356 (1966).
Bondi, H., Proc. Roy. Soc, A, 269, 21 (1962).
Kyle, M., and Bailey, J. A., Nature, 217, 907 (1968), (Paper 19).
Davies, J. G., Horton, P. W., Lyne, A. G., Rickett, B. J., and Smith, F. G., Nature, 217, 910 (1968), (Paper 6).
Author information
Authors and Affiliations
Rights and permissions
Copyright information
© 1968 Springer Science+Business Media New York
About this chapter
Cite this chapter
Saslaw, W.C., Faulkner, J., Strittmatter, P.A. (1968). Rapidly Pulsing Radio Sources. In: Pulsating Stars. Springer, Boston, MA. https://doi.org/10.1007/978-1-4899-6387-1_42
Download citation
DOI: https://doi.org/10.1007/978-1-4899-6387-1_42
Publisher Name: Springer, Boston, MA
Print ISBN: 978-1-4899-6191-4
Online ISBN: 978-1-4899-6387-1
eBook Packages: Springer Book Archive