Hostname: page-component-848d4c4894-5nwft Total loading time: 0 Render date: 2024-06-04T06:42:27.560Z Has data issue: false hasContentIssue false
  • English
  • Français

Pulsar Microstructure Quasi-Periodicity

Published online by Cambridge University Press:  14 August 2015

Valentin Boriakoff ,
Dale C. Ferguson  and
Gregory Slater
Valentin Boriakoff
Affiliation:
NAIC, Cornell University, Ithaca, NY
Dale C. Ferguson
Affiliation:
NAIC, Arecibo Observatory, Arecibo, PR
Gregory Slater
Affiliation:
Cornell University, Ithaca, NY

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.

Microstructure in pulsars occasionally has a quasi-periodic character with an average period of around 0.9 ms. A survey of this little known phenomenon (time characteristics, polarization, frequency behaviour, etc.) together with some new results are presented. Some physical interpretations (e.g. vibration of the neutron star, polar cap periodical sparking, standing wave pattern in the velocity of light cylinder model) are also presented.

Type
III. Radio Observations of Pulsars
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 199 - 204
Copyright
Copyright © Reidel 1981 

References

Backer, D.C.: 1973, Astrophys. J. 182, pp. 245–276.Google Scholar
Boriakoff, V.: 1973, “Pulsar Radiofrequency Observations with a Digital Pulsar Processor”, NAIC Publication No. 38, Cornell University.Google Scholar
Boriakoff, V.: 1976, Astrophys. J. Letters 208, pp. L43–L46.Google Scholar
Boriakoff, V.: 1980, submitted.Google Scholar
Boriakoff, V. and Jackson, B.: 1980, in preparation.Google Scholar
Cheng, A.F.: 1981, this volume.Google Scholar
Cordes, J.M.: 1976, Astrophys. J. 208, pp. 944–954.Google Scholar
Cordes, J.M. and Hankins, T.H.: 1977, Astrophys. J. 218, pp. 484–503.Google Scholar
Ferguson, D.C., Graham, D.A., Jones, B.B., Seiradakis, J.H., and Wielebinski, R.: 1976, Nature 260, pp. 25–27.Google Scholar
Ferguson, D.C. and Seiradakis, J.H.: 1978, Astron. Astrophys. 64, pp. 27–42.Google Scholar
Hankins, T.H.: 1971, Astrophys. J. 169, pp. 487–494.CrossRefGoogle Scholar
Hankins, T.H. and Boriakoff, V.: 1978, Nature 276, pp. 45–47.Google Scholar
Hankins, T.H. and Boriakoff, V.: 1980, Nature, in press.Google Scholar
Harding, A.K. and Tademaru, E.: 1979, Astrophys. J. 233, pp. 317–326.Google Scholar
Harding, A.K. and Tademaru, E.: 1980, Astrophys. J. 238, pp. 1054–1065.CrossRefGoogle Scholar
Harding, A.K. and Tademaru, E.: 1981, Astrophys. J., in press.Google Scholar
van Horn, H.M.: 1980, Astrophys. J. 236, pp. 899–903.Google Scholar
Ipser, J.R. and Thorne, K.S.: 1973, Astrophys. J. 181, pp. 181–182.Google Scholar
Kardashev, N.S., Kuzmin, A.D., Nikolaev, N.Ya., Novikov, A.Yu., Popov, M.V., Smirnova, T.V., Soglasnov, V.A., Shavanova, T.V., Shinskii, M.D., and Shitov, Yu.P.: 1978, Sov. Astron. 22 (5), pp. 583–587.Google Scholar