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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. 3.

Most likely values for ﹩V^{( P) }_{r}﹩ and z0 for four pulsars using three different values of braking index. Three lines are shown for each value of braking index to designate the peak likelihood and the 68% confidence regions. Heavy solid lines: n = 4. Light solid lines: n = 3. Long dashed lines: n = 2.5. Dotted lines: n = 2.

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