Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-08-23
Int.J.Mod.Phys.D14:1075-1082,2005
Astronomy and Astrophysics
Astrophysics
to appear in the International Journal of Modern Physics D
Scientific paper
10.1142/S0218271805006535
Two Galactic isolated strong X-ray pulsars seem to be in the densest environments compared to other types of Galactic pulsar. X-ray pulsar J1846-0258 can be in an early phase of anomalous X-ray pulsars and soft gamma repeaters if its average braking index is ~1.8-2.0. X-ray pulsar J1811-1925 must have a very large average braking index (n~11) if this pulsar was formed by SN 386AD. This X-ray pulsar can be in an early phase of evolution of the radio pulsars located in the region P~50-150 ms and \.{P}~10$^{-14}-10^{-16}$ s/s of the P-\.{P} diagram. X-ray/radio pulsar J0540-69 seems to be evolving in the direction to the dim isolated thermal neutron star region on the P-\.{P} diagram. Possible progenitors of different types of neutron star are also discussed.
Ankay Askin
Karanfil G.
Sahin S.
Yazgan Efe
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