Fig. 2 from Neutron Star Population Dynamics. II. Three‐dimensional Space Velocities of Young Pulsars

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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. 2.

Lines showing most likely values for ﹩V^{( P) }_{r}﹩ and z₀. For three pulsars (B0540+23, B1449−64, and B2224+65), dashed lines indicate the 68% confidence interval.

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