Evolutionary processes in Neutron Star Binaries

Details Evolutionary processes in Neutron Star Binaries Evolutionary processes in Neutron Star Binaries

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1379...31b&link_type=abstract

ASTROPHYSICS OF NEUTRON STARS 2010: A Conference in Honor of M. Ali Alpar. AIP Conference Proceedings, Volume 1379, pp. 31-34 (

Astronomy and Astrophysics

Astrophysics

Magnetic Fields, Stellar Winds, Accretion, X-Ray Binary Stars, Stellar Structure, Electric And Magnetic Fields, Solar Magnetism, Mass Loss And Stellar Winds, Accretion And Accretion Disks, X-Ray Binaries, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

Interaction with binary companion has profound effects on a neutron star. Magnetic interaction with the companion's stellar wind and accretion flow causes major changes in the spin rate, accretion on the star causes heating, changes crustal composition and reduces the magnetic field strength. This article reviews the various physical processes in the neutron star that accompany such changes.

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