On the evolution of pulsars

Details On the evolution of pulsars On the evolution of pulsars

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..408n&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, Mar.-Apr. 1985, p. 408-410) Soviet Astronomy (ISSN 0038-5301), vol. 29, Mar.-Apr. 1985, p. 2

Astronomy and Astrophysics

Astronomy

1

Pulsars, Stellar Evolution, Stellar Models, Magnetic Dipoles, Stellar Luminosity, Stellar Rotation

Scientific paper

On the basis of the analysis of published data the braking index n = 3.1±0.2 was estimated for pulsars whose total luminosity exceeds 2×1032erg/s and is less than 5×1035erg/s. Such an estimate of the braking index allows the suggestion that the evolution of the pulsars in question seems to proceed in accordance with the law describing the energy losses by a rotating magnetic dipole.

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