On the relationship between pulsars and supernova remnants

Details On the relationship between pulsars and supernova remnants On the relationship between pulsars and supernova remnants

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981japa....2...87k&link_type=abstract

Journal of Astrophysics and Astronomy, vol. 2, Mar. 1981, p. 87-93. Research supported by the Deutsche Forschungsgemeinschaft.

Astronomy and Astrophysics

Astronomy

1

Pulsars, Radio Emission, Supernova Remnants, Black Holes (Astronomy), Crab Nebula, Neutron Stars, Shock Waves, X Ray Spectra

Scientific paper

It is proposed that single stars in the mass range 4-6.5 solar masses, that explode as supernovae of Type I, are totally disrupted by the explosion and form shell-type remnants. More massive single stars which explode as supernovae of Type II also give rise to shell-type remnants, but in this case a neutron star or a black hole is left behind. The first supernova explosion in a close binary also gives rise to a shell-type supernova remnant. The Crab-like filled-center supernova remnants are formed by the second supernova explosion in a close binary. The hybrid supernova remnants, consisting of a filled center surrounded by a shell, are formed if there is an active neutron star inside the shell.

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