TEMPO2, a new pulsar timing package - II. The timing model and precision estimates Mon Not R Astron Soc, 372 (2006), pp. 1549-1574, 10.1111/j.1365-2966.2006.10870.x arXiv:astro-ph/0607664 View in ScopusGoogle Scholar [65] Ellis J.A., Vallisneri M., Taylor S.R., Baker P.T. ...
However, the estimated initial spin exists the bias based on the magnetic dipole radiation (MDR) model, since the braking index of a dozen of observed pulsars ranges in that is deviated from the expected value of 3 by MDR. The magnetic dipole radiation plus wind (MDRW) model for a pulsar...