Hostname: page-component-848d4c4894-nr4z6 Total loading time: 0 Render date: 2024-05-08T22:16:30.324Z Has data issue: false hasContentIssue false

The Magnetic Pole Model for Pulsar Emission

Published online by Cambridge University Press:  25 April 2016

R. N. Manchester*
Affiliation:
Division of Radiophysics, CSIRO, Sydney

Extract

Pulsars are unique astronomical objects in that their emission is in the form of a periodic pulse train. For most pulsars the pulse duty cycle is small, only a few per cent of the period. The shapes and intensities of individual pulses are in general quite variable. This is illustrated in Figure 1 which shows a series of individual pulses from PSR 1133 + 16. Despite this variation in shape of individual pulses, it is found that the mean or integrated pulse profile obtained by adding many pulses synchronously with the period is in most cases stable in shape.

Type
Invited Papers
Copyright
Copyright © Astronomical Society of Australia 1978

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Backer, D. C, Nature.11%, 1297 (1970).Google Scholar
Backer, D. C, Astrophys. J., 182, 245 (1973).Google Scholar
Bennett, K., Bignami, G. F., Boella, G., Buccheri, R., Hermsen, W., Kanbach, G., Lichti, G. G. Mansou, J. L., Mayer-Hasselwander, H. A., Paul, J. A., Scarsi, L., Swanenburg, B. N., Taylor, B. G., and Wills, R. D., Astron. Astrophys., 61, 279 (1977).Google Scholar
Buccheri, R., Caraveo, P., D’Amico, N., Hermsen, W., Kanbach, G., Lichti, G. G., Mansou, J. L., Wills, R. D., Manchester, R. N., and Newton, L. M., Astron. Astrophys. (submitted) (1978).Google Scholar
Craft, H. D., 1970, Cornell Center for Radiophysics and Space Research, Report 395.Google Scholar
Durdin, J. M., Large, M. I., Little, A. G., Manchester, R. N., Lyne, A. G., and Taylor, J. H., in preparation (1978).Google Scholar
Gold, T., Nature, 221, 25 (1969).Google Scholar
Jones, P. B., Astrophys. J., 209, 602 (1976).CrossRefGoogle Scholar
Kurfess, J. D., Astrophys. J., 168, L39 (1971).CrossRefGoogle Scholar
Manchester, R. N., Astrophys. J., 163, L61 (1971).Google Scholar
Manchester, R. N., Goss, W. M., Newton, L. M., and Hamilton, P. A., Proc. Astron. Soc. Aust., 3, 81 (1976).CrossRefGoogle Scholar
Manchester, R. N., and Lyne, A. G., Mon. Not. R. Astron. Soc, 181, 761 (1977).CrossRefGoogle Scholar
Manchester, R. N., Lyne, A. G., Goss, W. M., Smith, F. G., Disney, M. J., Hartley, K. F., Jones, D. H. P., Wellgate, G. B., Danziger, I. J., Murdin, P. G., Peterson, B. A., and Wallace, P. T., Mon. Not. R. Astron. Soc. (in press) (1978a).Google Scholar
Manchester, R. N., Lyne, A. G., Taylor, J. H., Durdin, J. M., Large, M. I., and Little, A. G., Mon. Not. R. Astron. Soc. (in press) (1978b).Google Scholar
Manchester, R. N., and Taylor, J. H., Pulsars, Freeman, San Francisco (1977).Google Scholar
Manchester, R. N., Taylor, J. H., and Huguenin, G. R., Astrophys. J., 196, 83 (1975).CrossRefGoogle Scholar
Radhakrishnan, V., and Cooke, D. J., Astrophys. Lett., 3, 225 (1969).Google Scholar
Radhakrishnan, V., Cooke, D. J., Komesaroff, M. M., and Morris, D., Nature, 221, 443 (1969).Google Scholar
Rappaport, S., Bradt, H., afld Mayer, W., Nature Phys. Sci., 229, 40 (1971).CrossRefGoogle Scholar
Ruderman, M. A., and Sutherland, P. G., Astrophys. J., 196, 51 (1975).Google Scholar
Taylor, J. H., Manchester, R. N., and Huguenin, G. R., Astrophys. J., 195, 513 (1975).Google Scholar
Thompson, D. J., Astrophys. J., 201, L117 (1975).Google Scholar
Wallace, P. T., Peterson, B. A., Murdin, P. G., Danziger, I. J., Manchester, R. N., Lyne, A. G., Goss, W. M., Smith, F. G., Disney, M. J., Hartley, K. F., Jones, D. H. P., and Wellgate, G. W., Nature, 266, 692 (1977).Google Scholar
Warner, B., Nather, R. E., and Macfarlane, M., Nature, 222, 233 (1969).Google Scholar