The age of pulsars and a phenomenological model of their evolution

Details The age of pulsars and a phenomenological model of their evolution The age of pulsars and a phenomenological model of their evolution

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..992n&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, Sept.-Oct. 1991, p. 992-998. In Russian.

Astronomy and Astrophysics

Astronomy

Pulsars, Stellar Evolution, Stellar Models, Magnetic Moments, Phenomenology, Stellar Luminosity

Scientific paper

A model for the evolution of pulsars is proposed. Using data for 292 pulsars, it is shown that variations of their period, the time derivative of the period, and the angle between the magnetic moment and spin fit into a self-consistent model, while the dependence of energy losses on the angle corresponds to losses through magnetodipole radiation.

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