Fig. 5 from Neutron Star Population Dynamics. II. Three‐dimensional Space Velocities of Young Pulsars

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution

Export to PDF PPT Format

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. 5.

Contour plots of the log likelihood function for the double–Gaussian component model (n_g = 2, n_h = 1) as a function of values for pairs of parameters and for two‐dimensional slices through the best‐fit model. Contours are spaced by log 2.

Other Images in This Article

Copyright and Terms & Conditions