Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985basi...13...12k&link_type=abstract
Astronomical Society of India, Bulletin, vol. 13, March 1985, p. 12-52.
Astronomy and Astrophysics
Astronomy
8
Milky Way Galaxy, Neutron Stars, Pulsars, Stellar Mass, Supernova Remnants, X Ray Binaries, Cosmic Rays, Galactic Nuclei, Gamma Ray Spectra, Infrared Spectra, Stellar Evolution, Stellar Magnetic Fields, Visible Spectrum
Scientific paper
An overview is given discussing the primary and alternative interpretations of neutron stars (the primary one being that they are born in supernova explosions of massive stars and observed as radio pulsars if isolated and as X-ray binaries if attached to a close companion). The main theoretical tools are examined and the arguments are outlined by which one derives a neutron star mass of 1.2 plus or minus 0. 2 solar masses, radius of 10 to the (1 + or - 0.2) km, surface magnetic field of 6 x 10 to the (12 + or - 0.5) G and pulsar age of several million years. Even in exotic sources like So X-1, SS 433, and Cyg X-1, the presence of a neutron star may well be indicated.
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