Hostname: page-component-7c8c6479df-fqc5m Total loading time: 0 Render date: 2024-03-28T15:18:07.342Z Has data issue: false hasContentIssue false

Pulsar Surveys

Published online by Cambridge University Press:  04 August 2017

R.N. Manchester*
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76, Epping, NSW 2121 Australia

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.

The current situation regarding pulsar surveys is briefly reviewed. Most of the known pulsars have been found by major radio surveys that were unbiased in the sense of more-or-less uniformly covering a given area of sky. The results from two recent such surveys, the Green Bank 390 MHz survey of Stokes et al. (1985) and the Jodrell Bank 1400 MHz survey of Clifton and Lyne (1986) are compared. Conclusions are drawn regarding the effect of observing frequency on the results of pulsar surveys and the galactic distribution of pulsars and interstellar electrons.

Type
I. Rotation-Powered Pulsars
Copyright
Copyright © Reidel 1987 

References

Backer, D.C., Kulkarni, S.R., Heiles, C., Davis, M.M., and Goss, W.M.: 1982, Nature 300, 615.Google Scholar
Boriakoff, V., Buccheri, R. and Fauci, F.: 1983, Nature 304, 417.CrossRefGoogle Scholar
Clifton, T.R., and Lyne, A.G.: 1986, Nature 320, 43.Google Scholar
Damashek, M., Taylor, J.H., and Hulse, R.A.: 1978, Astrophys. J. 225, L31.Google Scholar
Damashek, M., Taylor, J.H., Backus, P.R., and Burkhardt, R.: 1982, Astrophys. J. 253, L57.CrossRefGoogle Scholar
D'Amico, N., Manchester, R.N., Taylor, J.H., Stokes, G.H., Durdin, J.M., and Brissenden, R.J.V.: 1986 (in preparation).Google Scholar
Davies, J.G., Lyne, A.G., and Seiradakis, J.H.: 1972, Nature 240, 229.CrossRefGoogle Scholar
Davies, J.G., Lyne, A.G., and Seiradakis, J.H.: 1973, Nature Phys. Sci. 244, 84.Google Scholar
Dewey, R.J., Taylor, J.H., Weisberg, J.M., and Stokes, G.H.: 1985, Astrophys. J. 294, L25.Google Scholar
Hewish, A., Bell, S.J., Pilkington, D.H., Scott, P.F., and Collins, R.A.: 1968, Nature 217, 709.CrossRefGoogle Scholar
Hulse, R., and Taylor, J.H.: 1974, Astrophys. J. 191, L59.CrossRefGoogle Scholar
Hulse, R., and Taylor, J.H.: 1975, Astrophys. J. 195, L51.CrossRefGoogle Scholar
Kulkarni, S.R.: 1986, Astrophys. J. (in press).Google Scholar
Large, M.I., and Vaughan, A.E.: 1971, Mon. Not. R. Astron. Soc. 151, 277.Google Scholar
Lyne, A.G., Manchester, R.N., and Taylor, J.H.: 1985, Mon. Not. R. Astron Soc. 213, 613.CrossRefGoogle Scholar
McCulloch, P.M., Hamilton, P.A., Ables, J.G., and Hunt, A.J.: 1983, Nature 303, 307.Google Scholar
Manchester, R.N., Lyne, A.G., Taylor, J.H., Durdin, J.M., Large, M.I., and Little, A.G.: 1978, Mon. Not. R. Astron. Soc. 185, 409.Google Scholar
Manchester, R.N., D'Amico, N., and Tuohy, I.R.: 1985, Mon. Not. R. Astron. Soc. 212, 975.CrossRefGoogle Scholar
Segelstein, D.J., Rawley, L.A., Stinebring, D.R., Fruchter, A.S., and Taylor, J.H.: 1986, Nature (submitted).Google Scholar
Seward, F.D., and Harnden, F.R.: 1982, Astrophys. J. 256, L45.CrossRefGoogle Scholar
Seward, F.D., Harnden, F.R., and Helfand, D.J.: 1984, Astrophys. J. 287, L19.Google Scholar
Stokes, G.H., Taylor, J.H., Weisberg, J.M., and Dewey, R.J.: 1985, Nature 317, 787.Google Scholar
Stokes, G.H. Segelstein, D.J. Taylor, J.H., and Dewey, R.J.: 1986, Astrophys. J. (submitted).Google Scholar
Taylor, J.H., and Stinebring, D.R.: 1986, Annu. Rev. Astron. Astrophys. (in press).Google Scholar
van den Heuvel, E.P.J.: 1984, J. Astrophys. Astron. 5, 209.Google Scholar