Fig. 4 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. 4.

Contour plot of the log likelihood function for the single–Gaussian component model (n_g = 1, n_h = 1) as a function of the rms velocity and scale height. Contours are spaced by log 2.

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