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2010MNRAS.407.1090B - Mon. Not. R. Astron. Soc., 407, 1090-1097 (2010/September-2)
The evolution of isolated neutron stars until accretion: the role of the initial magnetic field.
BOLDIN P.A. and POPOV S.B.
Abstract (from CDS):
It is shown that though the subsonic propeller stage can be relatively long, initially highly magnetized neutron stars (B0≳ 1013G) reach the accretion regime within the Galactic lifetime if their kick velocities are not too large. The fact that in previous studies made >10 yr ago such objects were not considered results in a slight increase of the accretor fraction in comparison with earlier conclusions. Most of the neutron stars similar to the Magnificent Seven are expected to become accreting from the interstellar medium after a few billion years of their evolution. They are the main predecessors of accreting isolated neutron stars.
Abstract Copyright: © 2010 The Authors. Journal compilation © 2010 RAS
Journal keyword(s): stars: neutron - pulsars: general
Simbad objects: 3
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