Comparing models of the periodic variations in spin-down and beamwidth for PSR B1828−11-Reference-Cited by-同舟云学术

Comparing models of the periodic variations in spin-down and beamwidth for PSR B1828−11

Published:2016-02-23 Issue:1 Volume:458 Page:881-899
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Ashton G.,Jones D. I.,Prix R.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/458/1/881/8181740/stw334.pdf

Reference33 articles.

1. Precession of the isolated neutron star PSR B1828--11

2. Evolution of non-spherical pulsars with plasma-filled magnetospheres

3. Bailes M. Lyne A. G. Shemar S. L. ASP Conf. Ser. Vol. 36, Planets Around Pulsars. Phillips J. A. Thorsett S. E. Kulkarni S. R. , editors. Astron. Soc. Pac.; San Francisco; 1993. p. 19.

4. Cordes J. ASP Conf. Ser. Vol. 36, Planets Around Pulsars. Phillips J. A. Thorsett J. E. Kulkarni S. R. , editors. Astron. Soc. Pac.; San Francisco; 1993. p. 43.

5. PULSAR STATE SWITCHING FROM MARKOV TRANSITIONS AND STOCHASTIC RESONANCE

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