The neutron stars in supernova remnants

Details The neutron stars in supernova remnants The neutron stars in supernova remnants

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974azh....51.1197a&link_type=abstract

Astronomicheskii Zhurnal, vol. 51, Nov.-Dec. 1974, p. 1197-1203. In Russian.

Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Neutron Stars, Stellar Evolution, Stellar Magnetic Fields, Supernova Remnants, Binary Stars, Magnetic Flux, Pulsars, Radio Astronomy, Relativistic Particles, Synchrotron Radiation, X Ray Astronomy

Scientific paper

The data about supernova remnants are analyzed in order to investigate black holes. For the support of synchrotron radiation of remnants the magnetic field of remnants must be changed to a complex exponent of R, and the continuous injection of relativistic particles must take place. The energy of supernova remnants, the increase of magnetic flux, and the polarization data are suggested on the assumption that there is a neutron star (pulsar) in every supernova remnant. The remnants with the black holes do not radiate in radio. Research on black holes in binary systems is more promising.

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