Early phases of different types of isolated neutron star
| dc.creator | Ankay, A. | |
| dc.creator | Yazgan, E. | |
| dc.creator | Sahin, S. | |
| dc.creator | Karanfil, G. | |
| dc.date | 2004-08-23 | |
| dc.date | 2004-11-19 | |
| dc.date.accessioned | 2026-07-07T10:47:54Z | |
| dc.date.available | 2026-07-07T10:47:54Z | |
| dc.description | 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. | |
| dc.description | to appear in the International Journal of Modern Physics D | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0408401 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0408401 | |
| dc.identifier | Int.J.Mod.Phys.D14:1075-1082,2005 | |
| dc.identifier | doi:10.1142/S0218271805006535 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/183694 | |
| dc.subject | Astrophysics | |
| dc.title | Early phases of different types of isolated neutron star | |
| dc.type | text |