Neutron stars in supernova remnants

Details Neutron stars in supernova remnants Neutron stars in supernova remnants

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sva....18..712a&link_type=abstract

(Astronomicheskii Zhurnal, vol. 51, Nov.-Dec. 1974, p. 1197-1203.) Soviet Astronomy, vol. 18, May-June 1975, p. 712-716. Transl

Astronomy and Astrophysics

Astronomy

2

Black Holes (Astronomy), Neutron Stars, Stellar Evolution, Stellar Magnetic Fields, Supernova Remnants, Binary Stars, Energy Distribution, 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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