Hostname: page-component-848d4c4894-75dct Total loading time: 0 Render date: 2024-05-31T10:51:22.928Z Has data issue: false hasContentIssue false
  • English
  • Français

Finding Pulsars at Parkes

Published online by Cambridge University Press:  05 March 2013

R. N. Manchester
R. N. Manchester*
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia; rmanches@atnf.csiro.au
Rights & Permissions [Opens in a new window]

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.

There are many reasons why it is important to increase the number of known pulsars. Not only do pulsar searches continue to improve statistical estimates of, for example, pulsar birthrates, lifetimes and the Galactic distribution, but they continue to turn up interesting and, in some cases, unique individual pulsars. In the early days of pulsar astronomy, the Molonglo radio telescope led the world as a pulsar detection instrument. However, the Parkes radio telescope, with its frequency versatility and greater tracking ablility, combined with sensitive receivers and powerful computer detection algorithms, is now the world’s most successful telescope at finding pulsars. The Parkes multibeam survey, begun in 1997, by itself will come close to doubling the number of known pulsars. Parkes has also been very successful at finding millisecond pulsars (MSPs), especially in globular clusters. One third of the known MSPs have been found in just one cluster, 47 Tucanae.

Keywords

pulsars: generalsurveysISM: general
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 18 , Issue 1 , 2001 , pp. 1 - 11
Copyright
Copyright © Astronomical Society of Australia 2001

References

Alpar, M. A., Cheng, K. S., & Pines, D. 1989, ApJ, 346, 823 CrossRefGoogle Scholar
Anderson, S. B. 1992, PhD thesis, California Institute of Technology Google Scholar
Backer, D. C., Kulkarni, S. R., Heiles, C., Davis, M. M., & Goss, W. M. 1982, Nature, 300, 615 Google Scholar
Bhattacharya, D., & van den Heuvel, E. P. J. 1991, Phys. Rep., 203, 1 CrossRefGoogle Scholar
Camilo, F. M., et al. 2000a, ApJ, 541, 367 Google Scholar
Camilo, F., Lorimer, D. R., Freire, P., Lyne, A. G., & Manchester, R. N. 2000b, ApJ, 535, 975 CrossRefGoogle Scholar
Camilo, F., et al. 2001, ApJ, 548, L187 Google Scholar
Clifton, T. R., Lyne, A. G., Jones, A. W., McKenna, J., & Ashworth, M. 1992, MNRAS, 254, 177 CrossRefGoogle Scholar
Crawford, F., et al. 2001, ApJ, in pressGoogle Scholar
Edwards, R. T. 2000, in Pulsar Astronomy – 2000 and Beyond, IAU Colloqu. 177, ed. M. Kramer, N. Wex & R. Wielebinski (San Francisco: ASP), p. 33 Google Scholar
Frail, D. A., Weisberg, J. M., Cordes, J. M., & Mathers, C. 1994, ApJ, 436, 144 Google Scholar
Freire, P. C., Camilo, F., Lorimer, D. R., Lyne, A. G., & Manchester, R. N. 2000, in Pulsar Astronomy – 2000 and Beyond, IAU Colloqu. 177, ed. M. Kramer, N. Wex & R. Wielebinski (San Francisco: ASP), p. 87 Google Scholar
Fruchter, A. S., Stinebring, D. R., & Taylor, J. H. 1988, Nature, 333, 237 Google Scholar
Geffert, M., Hiesgen, M., Colin, J., Dauphole, B., & Ducourant, C. 1997, in Hipparcos – Venice '97, ESA Symp. 402, p. 579 Google Scholar
Gilliland, R. L., et al. 1998, ApJ, 507, 818 Google Scholar
Hamilton, T. T., Helfand, D. J., & Becker, R. H. 1985, AJ, 90, 606 CrossRefGoogle Scholar
Han, J. L., Manchester, R. N., & Qiao, G. J. 1999, MNRAS, 306, 371 CrossRefGoogle Scholar
Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., & Collins, R. A. 1968, Nature, 217, 709 Google Scholar
Hulse, R. A., & Taylor, J. H. 1974, ApJ, 191, L59 Google Scholar
Johnston, S., et al. 1992a, MNRAS, 255, 401 Google Scholar
Johnston, S., et al. 1992b, ApJ, 387, L37 CrossRefGoogle Scholar
Johnston, S., et al. 1993, Nature, 361, 613 Google Scholar
Johnston, S., et al. 1996, MNRAS, 279, 1026 Google Scholar
Kaspi, V. M., et al. 1994, ApJ, 423, L43 CrossRefGoogle Scholar
Kaspi, V. M. et al. 2000, ApJ, 543, 321 Google Scholar
Komesaroff, M. M., Ables, J. G., Cooke, D. J., Hamilton, P. A., & McCulloch, P. M. 1973, Astrophys. Lett., 15, 169 Google Scholar
Large, M. I., Vaughan, A. E., & Mills, B. Y. 1968, Nature, 220, 340 CrossRefGoogle Scholar
Large, M. I., Vaughan, A. E., & Wielebinski, R. 1968, Nature, 220, 753 Google Scholar
Lyne, A. G., Brinklow, A., Middleditch, J., Kulkarni, S. R., Backer, D. C., & Clifton, T. R. 1987, Nature, 328, 399 Google Scholar
Lyne, A. G., et al. 1998, MNRAS, 295, 743 Google Scholar
Lyne, A. G., et al. 2000, MNRAS, 312, 698 Google Scholar
McConnell, D., et al. 1991, MNRAS, 249, 654 Google Scholar
Manchester, R. N., et al. 1996, MNRAS, 279, 1235 Google Scholar
Manchester, R. N., Lyne, A. G., D'Amico, N., Johnston, S., Lim, J., & Kniffen, D. A. 1990, Nature, 345, 598 CrossRefGoogle Scholar
Manchester, R. N., Lyne, A. G., Robinson, C., D'Amico, N., Bailes, M., & Lim, J. 1991, Nature, 352, 219 CrossRefGoogle Scholar
Manchester, R. N., Lyne, A. G., Taylor, J. H., Durdin, J. M., Large, M. I., & Little, A. G. 1978, MNRAS, 185, 409 Google Scholar
Navarro, J., Manchester, R. N., Sandhu, J. S., Kulkarni, S. R., & Bailes, M. 1997, ApJ, 486, 1019 Google Scholar
Odenkirchen, M., Brosche, P., Geffert, M., & Tucholke, H. J. 1997, New Astron., 2, 477 CrossRefGoogle Scholar
Pivovaroff, M., Kaspi, V. M., & Camilo, F. 2000, ApJ, 535, 379 CrossRefGoogle Scholar
Radhakrishnan, V., Cooke, D. J., Komesaroff, M. M., & Morris, D. 1969, Nature, 221, 443 Google Scholar
Radhakrishnan, V., & Manchester, R. N. 1969, Nature, 222, 228 Google Scholar
Rasio, F. A., Pfahl, E. D., & Rappaport, S. 2000, ApJ, 532, 47 Google Scholar
Rickett, B. J. 1990, ARA&A, 28, 561 Google Scholar
Robinson, B. J., Cooper, B. F. C., Gardiner, F. F., Wielebinski, R., & Landecker, T. L. 1968, Nature, 218, 1143 Google Scholar
Robinson, C. R., Lyne, A. G., Manchester, A. G., Bailes, M., D'Amico, N., & Johnston, S. 1995, MNRAS, 274, 547 CrossRefGoogle Scholar
Sandhu, J. S., Bailes, M., Manchester, R. N., Navarro, J., Kulkarni, S. R., & Anderson, S. B. 1997, ApJ, 478, L95 CrossRefGoogle Scholar
Staelin, D. H., & Reifenstein, E. C. 1968, Science, 162, 1481 CrossRefGoogle Scholar
Stairs, I. H., et al. 2001, MNRAS, in pressGoogle Scholar
Staveley-Smith, L., et al. 1996, PASA, 13, 243 Google Scholar
Taylor, J. H., & Cordes, J. M. 1993, ApJ, 411, 674 Google Scholar
Taylor, J. H., Wolszczan, A., Damour, T., & Weisberg, J. M. 1992, Nature, 355, 132 Google Scholar
Wang, N., et al. 2000, MNRAS, in pressGoogle Scholar
Wolszczan, A., Kulkarni, S. R., Middleditch, J., Backer, D. C., Fruchter, A. S., & Dewey, R. J. 1989, Nature, 337, 531 CrossRefGoogle Scholar
Young, M. D., Manchester, R. N., & Johnston, S. 1999, Nature, 400, 848 Google Scholar