Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982afz....18..107m&link_type=abstract
(Astrofizika, vol. 18, Jan.-Mar. 1982, p. 107-118.) Astrophysics, vol. 18, no. 1, July 1982, p. 65-71. Translation.
Astronomy and Astrophysics
Astrophysics
8
Pulsars, Angular Distribution, Interstellar Gas, Magnetospheres, Neutron Stars, Periodic Variations, Pulse Duration, Stellar Mass Accretion
Scientific paper
The division of pulsars into two classes is investigated, and the observed differences between the parameters of these classes of pulsars are examined. Differences are found between short-period and long-period pulsars in the observed dependence of the width of the mean profile on the period, the variation of the position angle along the profile, and in a number of other properties. It is concluded that these observations can be explained by adopting the polar cap model for long-period pulsars and Smith's model for those with short periods.
Malov Igor F.
Suleimanova S. A.
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