Early neutron star evolution in high-mass X-ray binaries

13 Mar 2020 Ho Wynn C. G. Haverford Wijngaarden M. J. P. Southampton Andersson Nils Southampton Tauris Thomas M. Aarhus Haberl F. MPE

The application of standard accretion theory to observations of X-ray binaries provides valuable insights into neutron star properties, such as their spin period and magnetic field. However, most studies concentrate on relatively old systems, where the neutron star is in its late propeller, accretor, or nearly spin equilibrium phase... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • SOLAR AND STELLAR ASTROPHYSICS