Transformation of a Star into a Planet in a Millisecond Pulsar Binary-Reference-Cited by-同舟云学术

Transformation of a Star into a Planet in a Millisecond Pulsar Binary

Published:2011-09-23 Issue:6050 Volume:333 Page:1717-1720
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Bailes M.¹²,Bates S. D.³,Bhalerao V.⁴,Bhat N. D. R.¹,Burgay M.⁵,Burke-Spolaor S.⁶,D’Amico N.⁵⁷,Johnston S.⁶,Keith M. J.⁶,Kramer M.³⁸,Kulkarni S. R.⁴,Levin L.¹⁶,Lyne A. G.³,Milia S.⁵⁷,Possenti A.⁵,Spitler L.¹,Stappers B.³,van Straten W.¹

Affiliation:

1. Centre for Astrophysics and Supercomputing and ARC Centre for All-Sky Astrophysics (CAASTRO), Swinburne University of Technology, Post Office Box 218 Hawthorn, VIC 3122, Australia.

2. Department of Astronomy, University of California, Berkeley, CA 94720, USA.

3. Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK.

4. Caltech Optical Observatories, California Institute of Technology, MS 249-17, Pasadena, CA 91125, USA.

5. Istituto Nazionale di Astrofisica–Osservatorio Astronomico di Cagliari, Poggio dei Pini, 09012 Capoterra, Italy.

6. Australia Telescope National Facility, Commonwealth Scientific and Industrial Research Organisation (CSIRO) Astronomy and Space Science, Post Office Box 76, Epping NSW 1710, Australia.

7. Dipartimento di Fisica, Università degli Studi di Cagliari, Cittadella Universitaria, 09042 Monserrato (CA), Italy.

8. Max-Planck Institut für Radioastronomie, Auf dem Huegel 69, 53121 Bonn, Germany.

Abstract

Timing observations of a millisecond pulsar reveal a planet that is far denser than any known planet.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference29 articles.

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4. Formation of a single millisecond pulsar by the coalescence of a neutron star and a massive white dwarf;van den Heuvel E. P. J.;Astron. Astrophys.,1984

5. Discovery of a Young Radio Pulsar in a Relativistic Binary Orbit

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