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Planets Around Pulsars

Published online by Cambridge University Press:  25 May 2016

A. Wolszczan
A. Wolszczan*
Affiliation:
Penn State University, Dept. of Astronomy and Astrophysics 525 Davey Laboratory, University Park, PA 16802, U.S.A.

Abstract

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A discovery of three terrestrial-mass planets orbiting the millisecond pulsar PSR B1257+12 and a subsequent detection of the predicted effect of gravitational interaction between the two more massive planets confirms that the first extrasolar planetary system has been identified and that pulsars can be successfully used as probes of planetary dynamics. In the absence of detections of planet-sized objects around Sun-like stars, planets orbiting a precise pulsar clock represent a unique source of information concerning the origin and evolution of planetary systems.

Information

Type
4 Radio Pulsars
Information
Symposium - International Astronomical Union , Volume 165: Compact Stars in Binaries , 1996 , pp. 187 - 196
Copyright
Copyright © Kluwer 1996 

References

Bailes, M., Lyne, A.G. & Shemar, S.L. 1993, in Planets around Pulsars , Phillips, J.A., Thorsett, S.E. & Kulkarni, S.R. (Eds.), ASP Conf. Ser. 36, 19.Google Scholar
Bhattacharya, D. & Van den Heuvel, E.P.J. 1991, Phys. Rep. 203, 1.CrossRefGoogle Scholar
Demiański, M. & Prószyński, M. 1979, Nat 282, 383.CrossRefGoogle Scholar
Levy, E.H. 1993, in Planets around Pulsars , Phillips, J.A., Thorsett, S.E. & Kulkarni, S.R. (Eds.), ASP Conf. Ser. 36, 181.Google Scholar
Lyne, A.G. 1994, in Millisecond Pulsars: A Decade of Surprise , Fruchter, A.S., Tavani, M. & Backer, D.C. (Eds.), ASP Conf. Ser. (in press).Google Scholar
Malhotra, R. 1993, ApJ 407, 266.CrossRefGoogle Scholar
Malhotra, R., Black, D., Eck, A. & Jackson, A. 1992, Nat 356, 583.CrossRefGoogle Scholar
Nelder, J.A. & Mead, R. 1965, Computer J. 7, 308.CrossRefGoogle Scholar
Peale, S.J. 1993, AJ 105, 1562.CrossRefGoogle Scholar
Phinney, E.S. & Hansen, B.M.S. 1993, in Planets around Pulsars , Phillips, J.A., Thorsett, S.E. & Kulkarni, S.R. (Eds.), ASP Conf. Ser. 36, 371.Google Scholar
Podsiadlowski, P. 1993, in Planets around Pulsars , Phillips, J.A., Thorsett, S.E. & Kulkarni, S.R. (Eds.), ASP Conf. Ser. 36, 149.Google Scholar
Rasio, F.A. et al. 1992, Nat 355, 325.CrossRefGoogle Scholar
Rasio, F.A. et al. 1993, in Planets around Pulsars , Phillips, J.A., Thorsett, S.E. & Kulkarni, S.R. (Eds.), ASP Conf. Ser. 36, 107.Google Scholar
Ruden, S.P. 1993, in Planets around Pulsars , Phillips, J.A., Thorsett, S.E. & Kulkarni, S.R. (Eds.), ASP Conf. Ser. 36, 197.Google Scholar
Sargent, A.I. & Beckwith, S.V.W. 1993, Phys. Today 46, 22.CrossRefGoogle Scholar
Thorsett, S.E. & Dewey, R.J. 1993, ApJ 419, L65.CrossRefGoogle Scholar
Thorsett, S.E. et al. 1993, ApJ 405, L29.CrossRefGoogle Scholar
Wolszczan, A. 1991, Nat 350, 688.CrossRefGoogle Scholar
Wolszczan, A. 1994, Science 264, 538.CrossRefGoogle Scholar
Wolszczan, A. & Frail, D.A. 1992, Nat 355, 145.CrossRefGoogle Scholar
Woosley, S.E. 1987, in The Origin and Evolution of Neutron Stars , IAU Symp. 125, Helfand, D.J. & Huang, J.H. (Eds.), Reidel, p. 255.CrossRefGoogle Scholar