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  Advances in our understanding of the free precession candidate PSR B1828-11

Ashton, G., Jones, D. I., & Prix, R. (2017). Advances in our understanding of the free precession candidate PSR B1828-11. In Proceedings of Pulsar Astrophysics: The Next Fifty Years, IAU Symposium (pp. 307-308). doi:10.1017/S1743921317008249.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0001-7362-F Version Permalink: http://hdl.handle.net/21.11116/0000-0002-E812-4
Genre: Conference Paper

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 Creators:
Ashton, Gregory1, Author              
Jones, David Ian, Author
Prix, Reinhard1, 2, Author              
Affiliations:
1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              
2Searching for Continuous Gravitational Waves, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, Hannover, DE, ou_2630691              

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Free keywords: Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE
 Abstract: We highlight the advances and difficulties in understanding PSR B1828-11, which undergoes long-term periodic modulations in its timing and pulse shape over several years. A model comparison of precession and magnetospheric switching models based on the long-term modulation data favours the former; we discuss the implications of this in the context of short timescale switching observed in this pulsar. Furthermore, we highlight the difficulties this pulsar poses for our understanding of pulsars due to the increasing rate of the modulation period and its behaviour during a recent glitch.

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 Dates: 2018-01-1020182017
 Publication Status: Published in print
 Pages: 2
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 Identifiers: arXiv: 1801.03990
URI: http://arxiv.org/abs/1801.03990
DOI: 10.1017/S1743921317008249
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Title: Pulsar Astrophysics: The Next Fifty Years
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Title: Proceedings of Pulsar Astrophysics: The Next Fifty Years, IAU Symposium
Source Genre: Proceedings
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Pages: - Volume / Issue: 337 Sequence Number: - Start / End Page: 307 - 308 Identifier: -