Millisecond Radio Pulsars in 47 Tucanae
Astrophysics
2007-05-23 v1
Abstract
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.
Cite
@article{arxiv.astro-ph/0210460,
title = {Millisecond Radio Pulsars in 47 Tucanae},
author = {D. R. Lorimer and F. Camilo and P. Freire and M. Kramer and A. G. Lyne and R. N. Manchester and & N. D'Amico},
journal= {arXiv preprint arXiv:astro-ph/0210460},
year = {2007}
}
Comments
4 pages, 1 figure, to appear in proceedings of the conference "Radio Pulsars" held in Chania, Crete, Sept 2002