Image Details
Caption: Fig. 9.
Scatter plots of radial velocity ﹩V^{( P) }_{r}﹩ against birth altitude, z0, and perpendicular speed, V⊥, for three pulsars. The values result from the Monte Carlo solutions derived using eq. (32). Top row: B1953+50; Middle row: B2154+40; Bottom row: B2224+65.
© 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.