On the Connexion between Pulsars and Supernovae

Details On the Connexion between Pulsars and Supernovae On the Connexion between Pulsars and Supernovae

Jan 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970natur.225..438p&link_type=abstract

Nature, Volume 225, Issue 5231, pp. 438-439 (1970).

Physics

31

Scientific paper

I REPORT here some preliminary results of a statistical study of the spatial distribution of pulsars in the galaxy which have direct relevance to the pulsar-supernova hypothesis and to certain features in the observed distribution of pulsar galactic latitudes. I present evidence that most pulsars may have been formed in Type II supernova explosions and initially possessed extremely high velocities, of order 1,000 km s-1. On this basis, four new pulsar-supernova identifications are suggested.

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