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Millisecond Radio Pulsars in 47 Tucanae

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arxiv astro-ph/0210460 v1 pith:P6NZ73Y4 submitted 2002-10-21 astro-ph

D.R. Lorimer (JBO) , F. Camilo (Columbia) , P. Freire (NAIC) , M. Kramer (JBO) , A.G. Lyne (JBO) , R.N. Manchester (ATNF)& N.D'Amico (Cagliari Observatory) This is my paper · ORCID
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keywords clusterfreiremillisecondpulsarsradioreviewtucanaeahead
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We review the properties of the 22 millisecond radio pulsars currently known in the globular cluster 47 Tucanae, and their implications for the mass and gas content of the cluster. Further details can be found in the publications from this project to date (Camilo et al. 2000; Freire 2000; Freire et al. 2001a,b; Freire et al. 2003). Throughout the review, we look ahead to the future results anticipated from this fascinating cluster.

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  1. A new likely pulsar binary in 47~Tucanae from continuum searches

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    47 Tuc W41 is a redback millisecond-pulsar binary with Lx ~ 3e31 erg/s, steep-spectrum radio continuum, and an irradiated ~0.5 Msun secondary on a 10.4-hr orbit.

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