Dynamics of PSR J0045-7319/B-star Binary and Neutron Star Formation

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Recent timing observations have revealed the presence of orbital precession due to spin-orbit coupling and rapid orbital decay due to dynamical tidal interaction in the PSR J0045-7319/B-star binary system. They can be used to put concrete constraints on the age, initial spin and velocity of the neutron star.
latex (with sprocl.sty); 4 pages; To be published in 18th Texas Symposium on Relativistic Astrophysics (A. Olinto et al Ed.)

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