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Neutron Star Population Dynamics. II. Three‐dimensional Space Velocities of Young Pulsars

  • Authors: J. M. Cordes and David F. Chernoff

Cordes & Chernoff 1998 The Astrophysical Journal 505 315.

  • Provider: AAS Journals

Caption: Fig. 8.

One‐dimensional cuts through the likelihood functions for a double–Gaussian velocity PDF where the torque decay time τK is allowed to vary for different values of braking index. The heavy solid line for n = 2.5 yields the maximum likelihood solution at τK ~ 3 Myr. The two heavy dashed lines, for n = 4 and 4.5, yield the maximum likelihood if there is no decay, τK → ∞.

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