On the Characteristic and Dynamic Ages of Pulsars

Details On the Characteristic and Dynamic Ages of Pulsars On the Characteristic and Dynamic Ages of Pulsars

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap.....47...29m&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 47, Issue 1, p. 29-36 (2004).

Astronomy and Astrophysics

Astrophysics

Stars - Pulsars - Pulsars Ages

Scientific paper

A method that is independent of the model for the distribution of free electrons in the galaxy is proposed for revealing possible oscillations of pulsars in the direction perpendicular to the galactic plane. Oscillations of pulsars in this direction with a half period of approximately 108 years on the scale of characteristic ages are found by this method, which is independent of the distance scale.

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