Sushan Konar
Published 2017-09-21Version 1
This article briefly reviews our current understanding of the evolution of magnetic fields in neutron stars, which basically defines the evolutionary pathways between different observational classes of neutron stars. The emphasis here is on the evolution in binary systems and the newly emergent classes of millisecond pulsars.
Comments: Has appeared in Journal of Astrophysics and Astronomy special issue on 'Physics of Neutron Stars and Related Objects', celebrating the 75th birth-year of G. Srinivasan
Journal: J. Astrophys. Astr. 38(3) 47 (2017)
Neutron Stars in Supernovae and Their Remnants
Optical Astrometry of Accreting Black Holes and Neutron Stars: Scientific Opportunities
The role of $r$-mode damping in the thermal evolution of neutron stars
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