Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-20T09:16:14.993Z Has data issue: false hasContentIssue false
  • English
  • Français

Timing of Optical Pulses from the Crab Nebula Pulsar∗

Published online by Cambridge University Press:  07 February 2017

P. E. Boynton ,
E. J. Groth ,
R. B. Partridge  and
David T. Wilkinson
P. E. Boynton
Affiliation:
Joseph Henry Laboratories, Physics Department, Princeton University, Princeton, N.J., U.S.A.
E. J. Groth
Affiliation:
Joseph Henry Laboratories, Physics Department, Princeton University, Princeton, N.J., U.S.A.
R. B. Partridge
Affiliation:
Joseph Henry Laboratories, Physics Department, Princeton University, Princeton, N.J., U.S.A.
David T. Wilkinson
Affiliation:
Joseph Henry Laboratories, Physics Department, Princeton University, Princeton, N.J., U.S.A.

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.

Timing the arrival of optical pulses from NP 0532 is a potentially important tool for studying the physics of this fascinating object. However, there are some difficulties in interpreting the data in terms of physical models. Some progress has been made on understanding the largest effect – the pulsar braking mechanism. The glitch of late September, 1969 can be interpreted as the speed-up, and subsequent relaxation, of the rotation of a neutron star crust. An alternate explanation is that of a planet in an eccentric orbit. Both models fit the rather meager data near the event. A small sinusoidal effect is indicated in a relatively quiet period of the data.

Type
Session 2
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 119 - 124
Copyright
Copyright © Reidel 1971 

References

Baym, G., Pethick, C., Pines, D., and Ruderman, M.: 1969, Nature 224, 872.CrossRefGoogle Scholar
Boynton, P. E., Groth, E. J., Partridge, R. B., and Wilkinson, D. T.: 1969a, Astrophys. J. Letters 157, L197.CrossRefGoogle Scholar
Boynton, P. E., Groth, E. J., Partridge, R. B., and Wilkinson, D. T.: 1969b, IAU Circ. No. 2179.Google Scholar
Duthie, J. G., Murdin, P.: 1970, preprint.Google Scholar
Ginzburg, V. L. and Kirzhnits, D. A.: 1965, Soviet Phys. – JETP 20, 1346.Google Scholar
Gold, T.: 1968, Nature 218, 731.CrossRefGoogle Scholar
Greenstein, G. S. and Cameron, A. G. W.: 1969, Nature 222, 862.CrossRefGoogle Scholar
Gunn, J. E. and Ostriker, J. P.: 1969, Nature 221, 454.CrossRefGoogle Scholar
Hills, J. G.: 1970, Nature 226, 730.CrossRefGoogle Scholar
Hoffman, B.: 1968, Nature 218, 667.CrossRefGoogle Scholar
Michel, F. C.: 1970, Astrophys. J. Letters 159, L25.CrossRefGoogle Scholar
Migdal, A. B.: 1960, Soviet Phys. – JETP 10, 176.Google Scholar
Nelson, J., Hills, R., Cudaback, D., and Wampler, J.: 1970, Astrophys. J. Letters 161, L235.CrossRefGoogle Scholar
Pacini, F.: 1967, Nature 216, 567.CrossRefGoogle Scholar
Richards, D. W. and Comella, J. M.: 1969, Nature 222, 552.Google Scholar
Richards, D. W., Pettengill, G. H., Counselman, C. C., and Rankin, J. M.: 1970, Astrophys. J. Letters 160, L1.CrossRefGoogle Scholar
Richards, D. W., Pettengill, G. H., Roberts, J. A., Counselman, C. C., and Rankin, J.: 1969, IAU Circ. No. 2181.Google Scholar
Ruderman, M.: 1969, Nature 223, 597.CrossRefGoogle Scholar
Ruderman, M.: 1970, Nature 225, 838.CrossRefGoogle Scholar