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Scenarios for the formation of binary and millisecond pulsars – A critical assessment

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Abstract

The evolution of high-and low-mass X-ray binaries (HMXB and LMXB) into different types of binary radio pulsars, the ‘high-mass binary pulsars’(HMBP) and ‘low-mass binary pulsars’ (LMBP) is discussed. The HMXB evolve either into Thorne-Zytkow objects or into short-period binaries consisting of a helium star plus a neutron star (or a black hole), resembling Cygnus X-3. The latter systems evolve (with or without a second common-envelope phase) into close binary pulsars, in which the companion of the pulsar may be a massive white dwarf, a neutron star or a black hole ( some final systems may also consist of two black holes). A considerable fraction of the systems may also be disrupted in the second supernova explosion. We discuss the possible reasons why the observed numbers of double neutron stars and of systems like Cyg X-3 are several orders of magnitude lower than theoretically predicted. It is argued that the observed systems form the tip of an iceberg of much larger populations of unobserved systems, some of which may become observable in the future. As to the LMBP, we consider in some detail the origins of systems with orbital periods in the range 1–20 days. We show that to explain their existence, losses of orbital angular momentum (e.g., by magnetic braking) and in a number of cases: also of mass, have to be taken into account. The masses of the low-mass white dwarf companions in these systems can be predicted accurately. We notice a clear correlation between spin period and orbital period for these systems, as well as a clear correlation between pulsar magnetic field strength and orbital period. These relations strongly suggest that increased amounts of mass accreted by the neutron stars lead to increased decay of their magnetic fields: we suggest a simple way to understand the observed value of the ‘bottom’ field strengths of a few times 108 G. Furthermore, we find that the LMBP-systems in which the pulsar has a strong magnetic field (> 1011 G) have an about two orders of magnitude larger birth rate (i.e., about 4 × 10-4 yr-1 in the Galaxy) than the systems with millisecond pulsars (which have B < 109 G). Using the observational fact that neutron stars receive a velocity kick of ∼450 km/s at birth, we find that some 90% of the potential progenitor systems of the strong-field LMBP must have been disrupted in the Supernovae in which their neutron stars were formed. Hence, the formation rate of the progenitors of the strong-field LMBP is of the same order as the galactic supernova rate (4 × 10-3 yr-1). This implies that a large fraction of all Supernovae take place in binaries with a close low-mass (< 2.3 M⊙) companion.

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References

  • Abbott, D.C. and Conti, P.S. 1987,Ann. Rev. Astron. Astrophys.,25, 113.

    Article  ADS  Google Scholar 

  • Alpar, M.A., Cheng, A.F., Ruderman, M. and Shaham, J. 1982,Nature,300, 728

    Article  ADS  Google Scholar 

  • Bailes, M., Harrison, P.A., Lorimer, D.R., Johnston, S., Lyne, A.G., Manchester, R.N., D’Amico, N., Nicastro, L., Tauris, T. and Robinson, C. 1994,Astrophys. J.,425, L41.

    Article  ADS  Google Scholar 

  • Baylin, C D. and Grindlay, J.E. 1990,Astrophys. J, 353, 159.

    Article  ADS  Google Scholar 

  • Bhattacharya, D. and Van den Heuvel, E.P.J. 1991,Phys. Reports,203, 1.

    Article  ADS  Google Scholar 

  • Bisnovatyi-Kogan, G.S. and Komberg, B.V. 1974,Astron. Zh.,51, 373(Soviet Astron. 18,217)

    ADS  Google Scholar 

  • Canal, R., Isern, J. and Labay, J. 1990,Ann. Rev. Astron. Astrophys. 28, 183.

    Article  ADS  Google Scholar 

  • Chen, K. and Ruderman, M. 1993,Astrophys. J.,408, 179.

    Article  ADS  Google Scholar 

  • Delgado, A.J. and Thomas, H.C. 1981,Astron. Astrophys. 96, 142.

    ADS  Google Scholar 

  • De Loore, C., De Grève, J.P. and De Cuyper, J.P. 1975,Astrophys. & Space Sci 36, 219.

    Article  ADS  Google Scholar 

  • Flannery, B.P. and Van den Heuvel, E.P.J. 1975,Astron. Astrophys.,39, 61.

    ADS  Google Scholar 

  • Foster, R.S., Wolszczan, A. and Camilo, F. 1993,Astrophys. J.,410, L91

    Article  ADS  Google Scholar 

  • Habets, G.M.H.J. 1985,Advanced Evolution of Helium Stars and Massive Close Binaries, Ph.D. Thesis, Univ. Amsterdam.

  • Habets, H.GJ.M. 1986,Astron. Astrophys.,187, 209.

    Google Scholar 

  • Hameury, J.-M., King, A.R., Lasota, J.P. and Raison, F. 1993,Astron. Astrophys.,277, 81.

    ADS  Google Scholar 

  • Harpaz, A. and Rappaport, S. 1991,Astrophys. J.,383, 739.

    Article  ADS  Google Scholar 

  • Hogeveen, S. 1991,The Mass Ratio Distribution of Binary Stars, Ph.D. Thesis, Univ. Amsterdam.

  • Hogeveen, S. 1992,Astrophys. & Space Sci.,196, 299.

    Article  ADS  Google Scholar 

  • Joss, P.C. and Rappaport, S. 1983,Nature,304, 419.

    Article  ADS  Google Scholar 

  • Joss, P.C., Rappaport, S. and Lewis, W. 1987,Astrophys. J.,319, 180.

    Article  ADS  Google Scholar 

  • Kippenhahn, R., Kohl, K. and Weigert, A. 1967,Zeitschr. f. Astrophysik,66, 58.

    ADS  Google Scholar 

  • Lipunov, A. 1992,Astrophysics of Neutron Stars (Springer).

  • Lipunov, A. 1992, inEvolutionary Relations in the Zoo of Interacting Binaries, Ed. F. d’Antona,Mem. Soc. Astron. Ital., (in press).

  • Lyne, A. and Lorimer, D. 1994,Nature,369, 127.

    Article  ADS  Google Scholar 

  • Meurs, E.M. and Van den Heuvel, E.P.J. 1989,Astron. Astrophys.,226, 88.

    ADS  Google Scholar 

  • Narayan, R., Piran, T. and Shemi, A. 1991,Astrophys. J.,379, L17.

    Article  ADS  Google Scholar 

  • Nice, D.J., Taylor, J.H. and Fruchter, A.S. 1993,Astrophys. J.,402, L49

    Article  ADS  Google Scholar 

  • Paczynski, B. 1971,Ann. Rev. Astron. Astrophys.,9, 183.

    Article  ADS  Google Scholar 

  • Paczunski, B. 1983,Nature,304, 421

    Article  ADS  Google Scholar 

  • Phinney, E.S. 1991,Astrophys. J.,380, L17.

    Article  ADS  Google Scholar 

  • Podsiadlowski, P. 1991,Nature,350, 136.

    Article  ADS  Google Scholar 

  • Pylyser, E. and Savonije, G.J. 1988,Astron. & Astrophys.,191, 57.

    ADS  Google Scholar 

  • Pylyser, E. and Savonije, G.J. 1989,Astron. & Astrophys.,208, 52.

    ADS  Google Scholar 

  • Radhakrishnan, V. and Srinivasan, G. 1982,Curr. Sci.,51, 1096

    ADS  Google Scholar 

  • Radhakrishnan, V. and Srinivasan, G. 1984, Proc. 2nd Asian-Pacific Regional Meeting of the IAU (eds. B. Hidayat and M.W. Feast), Jakarta, Tira Pustaka, p. 423.

    Google Scholar 

  • Refsdal, S. and Weigert, A. 1971,Astron. & Astrophys.,6, 426.

    ADS  Google Scholar 

  • Romani, R. 1990,Nature,347, 741.

    Article  ADS  Google Scholar 

  • Savonije, G.J. 1983,Nature,304, 422

    Article  ADS  Google Scholar 

  • Savonije, G.J. 1983, inAccretion Driven Stellar X-ray Sources, Eds, W.H.G. Lewin and E.P.J, van den Heuvel, (Cambridge Univ. Press), p. 343.

  • Smarr, L.L. and Blandford, R.D. 1976,Astrophys. J.,207, 574

    Article  ADS  Google Scholar 

  • Srinivasan, G. and Van den Heuvel, E.P.J. 1982,Astron. & Astrophys.,108, 143

    ADS  Google Scholar 

  • Stokes, G.H., Segelstein, D.J., Taylor, J.H. and Dewey, R.J. 1986,Astrophys. J.,311, 694.

    Article  ADS  Google Scholar 

  • Taam, R.E. 1983,Astrophys. J.,270, 694.

    Article  ADS  Google Scholar 

  • Taam, R.E. and Bodenheimer, P. 1992, inX-ray Binaries and Recycled Pulsars, Eds. E.P.J. van den Heuvel and S.A. Rappaport (Kluwer), p. 281.

  • Taam, R.E., Bodenheimer, P. and Ostriker, J.P. 1978,Astrophys. J.,222, 269.

    Article  ADS  Google Scholar 

  • Taylor, J.H., Manchester, R.N. and Lyne, A.G. 1993,Astrophys. J. Supp.,88, 529.

    Article  ADS  Google Scholar 

  • Tout, C. 1991,Monthly Notices Roy. Astron. Soc,250, 701.

    ADS  Google Scholar 

  • Tutukov, A.V. and Yungelson, L.R. 1993,Monthly Notices Roy. Astron. Soc,260, 675.

    ADS  Google Scholar 

  • Van den Heuvel, E.P.J. 1981a, inFundamental Problems in the Theory of Stellar Evolution, Ed. J. Sugimotoet al., (Reidel), p. 155.

  • Van den Heuvel, E.P.J. 1981b, inPulsars, Eds. W. Sieber and R. Wielebinski, (Reidel), p. 379.

  • Van den Heuvel, E.P.J. 1983, inAccretion Driven Stellar X-ray Sources, Eds. W.H.G. Lewin and E.P.J. van den Heuvel, (Cambridge Univ. Press), p. 303.

  • Van den Heuvel, E.P.J. 1992, inX-ray Binaries and Recycled Pulsars, Eds. E.P.J. van den Heuvel and S.A. Rappaport (Kluwer), p. 233.

  • Van den Heuvel, E.P.J. 1994, inInteracting Binaries, Lecture Notes Saas Fee Advanced Course 22, (Springer), p. 263.

  • Van den Heuvel, E.P.J. and Bitzaraki, O. 1994, inEvolutionary Relations in the Zoo of Interacting Binaries, Ed. F. d’Antona, Mem. Soc. Astron. Ital. (in press).

  • Van den Heuvel, E.P.J. and De Loore, C. 1973,Astron. & Astrophys.,25, 387

    ADS  Google Scholar 

  • Van den Heuvel, E.P.J. and Taam, R.E. 1984,Nature,309, 235.

    Article  ADS  Google Scholar 

  • Van der Hucht, K.A. 1992,Astron. Astrophys. Rev.,4, 123.

    Article  ADS  Google Scholar 

  • Van Kerkwijk, M.H. 1993,The Mass of VelaX-l, the Nature of Cygnus X-3, the Character of Be Stars, Ph.D. Thesis Univ. Amsterdam.

  • Van Paradijs, J. 1994, inX-ray Binaries, Eds W.H.G. Lewin, J. van Paradijs and E.P.J. van den Heuvel, (Cambridge Univ. Press), in press.

  • Verbunt, F. 1990, inNeutron Stars and their Birth Events, Ed. W. Kundt, (Kluwer), p. 179.

  • Verbunt, F. 1993,Ann. Rev. Astron. Astrophys.,31, 93.

    Article  ADS  Google Scholar 

  • Verbunt, F. and Zwaan, C. 1981,Astron. Astrophys.,100, L7.

    ADS  Google Scholar 

  • Webbink, R.F., Rappaport, S.A. and Savonije, G.J. 1983,Astrophys. J.,270, 678.

    Article  ADS  Google Scholar 

Download references

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  1. Astronomical Institute ‘Anton Pannekoek’, University of Amsterdam & Center for High-Energy Astrophysics, Amsterdam, The Netherlands

    E. P. J. van den Heuvel

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van den Heuvel, E.P.J. Scenarios for the formation of binary and millisecond pulsars – A critical assessment. J Astrophys Astron 16, 255–288 (1995). https://doi.org/10.1007/BF02714839

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