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Formation of Binary and Millisecond Pulsars: Puzzles and Possible Solutions

Published online by Cambridge University Press:  20 March 2013

Yong Shao  and
Xiang-Dong Li
Yong Shao
Affiliation:
Department of Astronomy and Key laboratory of Modern Astronomy and Astrophysics, Nanjing University, Nanjing 210093, China
Xiang-Dong Li
Affiliation:
Department of Astronomy and Key laboratory of Modern Astronomy and Astrophysics, Nanjing University, Nanjing 210093, China
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Abstract

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We present a systematic study of the evolution of intermediate- and low-mass X-ray binaries. Our calculations suggest that millisecond binary pulsars in wide orbits might have neutron stars born massive, or been formed through mass transfer driven by planet/brown dwarf-involved common envelope evolution.

Keywords

stars: millisecond pulsarsstars: evolutionMSPs: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 499 - 501
Copyright
Copyright © International Astronomical Union 2013

References

Bhattacharya, D. & van den Heuvel, E. P. J. 1991, Phys. Rev., 203, 1Google Scholar
Rappaport, S. A., et al. 1995, MNRAS, 273, 731Google Scholar
Shao, Y. & Li, X.-D. 2012 ApJ, 756, 85CrossRefGoogle Scholar
Tauris, T. M. 1996, A&A, 315, 453Google Scholar