Inner core wobble and free core nutation of pulsar PSR B1828-11

Author:

Kitiashvili I.,Gusev A.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference38 articles.

1. On the fast recovery of the Vela pulsar from its Christmas 1988 glitch;Alpar;Nature,1990

2. Barkin, Yu.V. Orbits rotation and formation of planets and satellites, in: Proceedings of the International Conference. “Geon-2003”. Kazan, Russia, pp. 15–21, 2003.

3. Cordes, J.M. ASP Conf. Ser. 36, Planets around Pulsars, In: J.A. Phillips, S.E. Thorsett, S.R. Kulkarni (Eds.), San Francisco: ASP, 43, 1993.

4. The crustal rigidity of a neutron star and implications for PSR 1828-11 and other precession candidates;Cutler;ApJ,2003

5. Can a solid inner core of Mars be detected from observations of polar motion and nutation of Mars?;Dehant;J. Geophys. Res.,2003

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