A Radio Pulsar/X-ray Binary Link

Author:

Archibald Anne M.1,Stairs Ingrid H.234,Ransom Scott M.5,Kaspi Victoria M.1,Kondratiev Vladislav I.567,Lorimer Duncan R.68,McLaughlin Maura A.68,Boyles Jason68,Hessels Jason W. T.910,Lynch Ryan11,van Leeuwen Joeri910,Roberts Mallory S. E.12,Jenet Frederick13,Champion David J.3,Rosen Rachel8,Barlow Brad N.14,Dunlap Bart H.14,Remillard Ronald A.15

Affiliation:

1. Department of Physics, McGill University, 3600 Rue University, Montréal, Quebec, H3A 2T8, Canada.

2. Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia V6T 1Z1, Canada.

3. Australia Telescope National Facility, Commonwealth Scientific and Industrial Research Organisation (CSIRO), Post Office Box 76, Epping, New South Wales 1710, Australia.

4. Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Mail 39, Post Office Box 218, Hawthorn Vic 3122, Australia.

5. National Radio Astronomy Observatory (NRAO), 520 Edgemont Road, Charlottesville, VA 22901, USA.

6. Department of Physics, West Virginia University, 210 Hodges Hall, Morgantown, WV 26506, USA.

7. Astro Space Center of the Lebedev Physical Institute, Profsoyuznaya 84/32, Moscow 117997, Russia.

8. National Radio Astronomy Observatory, Green Bank, WV 24944, USA.

9. Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA Dwingeloo, Netherlands.

10. Astronomical Institute Anton Pannekoek, University of Amsterdam, Kruislaan 403, 1098 SJ, Amsterdam, Netherlands.

11. Department of Astronomy, University of Virginia, Charlottesville, VA 22904–4325, USA.

12. Eureka Scientific, 2452 Delmer Street, Suite 100, Oakland, CA 94602-3017, USA.

13. Department of Physics and Astronomy, University of Texas at Brownsville, 80 Fort Brown, Brownsville, TX 78520, USA.

14. Department of Physics and Astronomy, University of North Carolina at Chapel Hill, CB 3255, Phillips Hall, Chapel Hill, NC 27599–3255, USA.

15. Massachusetts Institute of Technology Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, 37-287, Cambridge, MA 02139, USA.

Abstract

From X-ray Binary to Pulsar Pulsars with millisecond rotational periods are thought to originate from neutron stars in low-mass x-ray binaries that had their spin frequencies increased by long-lasting mass transfer from their companion stars. Using data from a radio pulsar survey, Archibald et al. (p. 1411 , published online 21 May; see the Perspective by Kramer ) found a neutron star in a low-mass X-ray binary that is in the process of turning into a radio millisecond pulsar. The system, which consists of a solar-like star and a 1.69-millisecond radio pulsar, has gone through a recent accretion phase, characteristic of low-mass X-ray binaries, but it shows no accretion disk anymore, confirming the evolutionary connection between millisecond radio pulsars and low-mass X-ray binaries.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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