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Do We Expect to See Young Pulsars outside Their Parent Shells?

Published online by Cambridge University Press:  25 April 2016

B. M. Gaensler  and
Simon Johnston
B. M. Gaensler
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, Australia. [email protected]
Simon Johnston
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, Australia. [email protected]
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Abstract

A recent study has indicated that a substantial fraction of young pulsars born in supernovae have travelled outside the boundaries of their corresponding shell supernova remnants. A simple model suggests that this should not be the case, implying either that some postulated pulsar/remnant associations are false, or that pulsars are particularly difficult to detect until they have emerged from their remnants.

Keywords

starsstatistics — starspulsarsgeneral — starssupernovaegeneral
Type
Gallactic and Stellar
Information
Publications of the Astronomical Society of Australia , Volume 12 , Issue 1 , April 1995 , pp. 76 - 80
Copyright
Copyright © Astronomical Society of Australia 1995

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References

Baade, W., & Zwicky, F. 1934, Proc. Nat. Acad. Sci., 20, 254 Google Scholar
Bailes, M., & Johnston, S. 1993, in Review of Radio Science, ed. Stone, W. R. (in Review of Radio Science, ed. Stone, W. R.: Oxford University Press), 677 Google Scholar
Bhattacharya, D. 1990, JA&A, 11, 125 Google Scholar
Caraveo, P. A. 1993, ApJ, 415, L111 Google Scholar
Fabian, A. C., Brinkmann, W., & Stewart, G. C. 1983, in IAU Symp. 101, Supernova Remnants and Their X-Ray Emission, eds Danziger, J. & Gorenstein, P. (Dordrecht: Reidel), 421 Google Scholar
Frail, D. A., Goss, W. M., & Whiteoak, J. B. Z. 1994, ApJ, 437, 781(FAW)Google Scholar
Frail, D. A., & Kulkarni, S. R. 1991, Nature, 352, 785 CrossRefGoogle Scholar
Frail, D. A., Kulkarni, S. R., & Vasisht, G. 1993, Nature, 365, 136 Google Scholar
Gull, S. F. 1973, MNRAS, 161, 47 Google Scholar
Harrison, P. A., Lyne, A. G., & Anderson, B. 1993, MNRAS, 261, 113 Google Scholar
Johnston, S., Manchester, R. N., Lyne, A. G., Kaspi, V. M., & D’Amico, N. 1995, A&A, 293, 795 Google Scholar
Kaspi, V. M., Lyne, A. G., Manchester, R. N., Johnston, S., D’Amico, N., & Shemar, S. L. 1993, ApJ, 409, L57 Google Scholar
Kassim, N. E., & Weiler, K. W. 1990, Nature, 343, 146 Google Scholar
Koribalski, B. S., Johnston, S., Weisberg, J., & Wilson, W. 1995, ApJ, 441, 756 Google Scholar
Large, M. I., Vaughan, A. E., & Mills, B. Y. 1968, Nature, 220, 340 Google Scholar
Lozinskaya, T. A. 1980, SvA, 24, 407 Google Scholar
Lyne, A. G., & Lorimer, D. R. 1994, Nature, 369, 127 Google Scholar
Lyne, A. G., Anderson, B., & Salter, M. J. 1982, MNRAS, 201, 503 CrossRefGoogle Scholar
McAdam, W.B., Osborne, J. L., & Parkinson, M. L. 1993, Nature, 361, 516 Google Scholar
McKee, C.F., & Ostriker, J. P. 1977, ApJ, 218, 148 CrossRefGoogle Scholar
Manchester, R. N., Kaspi, V. M., Johnston, S., Lyne, A. G., & D’Amico, N. 1991, MNRAS, 253, 7PGoogle Scholar
Radhakrishnan, V., & Srinivasan, G. 1980, JA&A, 1, 47 Google Scholar
Seward, F. D., & Harnden, F. R. 1982, ApJ, 256, L45 Google Scholar
Shull, J. M., Fesen, R. A., & Saken, J. M. 1989, ApJ, 346, 860 Google Scholar
Srinivasan, G., Bhattacharya, D., & Dwarakanath, K. S. 1984, JA&A, 5, 403 Google Scholar
Staelin, D. H., & Reifenstein, E.C. III 1968, Science, 162, 1481 Google Scholar
White, R. L., & Long, K. S. 1983, ApJ, 264, 196 Google Scholar