Spin Evolution of the Progenitors of Binary and Millisecond Pulsars
1996 ◽
Vol 165
◽
pp. 57-64
Keyword(s):
In this symposium, I have been given the task of summarizing our current understanding of the evolutionary history of spin periods of the neutron stars that we now see as binary and millisecond pulsars, i.e., recycled pulsars. We believe that a newborn, fast-spinning neutron star (with a rather high magnetic field ∼1011–1013 G) in a binary system first operates as a spin-powered pulsar, subsequently as an accretion-powered pulsar when accretion begins after the pulsar has been spun down adequately, and finally as a spin-powered pulsar for the second time after having been recycled to become a very fast-rotating neutron star (with a rather low magnetic field ∼108–1011 G) (see Ghosh 1994a, b, hereafter G94a, b).
2020 ◽
Vol 499
(3)
◽
pp. 3243-3254
Keyword(s):
2017 ◽
Vol 13
(S337)
◽
pp. 213-216
Keyword(s):
1992 ◽
Vol 128
◽
pp. 220-221
Keyword(s):
2018 ◽
Vol 480
(1)
◽
pp. 692-696
◽
2000 ◽
Vol 177
◽
pp. 619-620
◽
Keyword(s):
2019 ◽
Vol 36
◽
Keyword(s):
2017 ◽
Vol 45
◽
pp. 1760032
Keyword(s):