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Evolution of High-mass X-ray binaries in the Small Magellanic Cloud
| Content Provider | Scilit |
|---|---|
| Author | Yang, Jun Wik, Daniel R. |
| Copyright Year | 2018 |
| Description | In order to understand the progenitor of rotation powered pulsars, we compare them with High-mass X-ray binary (HMXB) pulsars, (or X-ray pulsars), in the Small Magellanic Cloud. The plot of period period vs. period derivative shows that isolated neutron stars could be evolved from HMXBs. The pulsars with long spin period might spin up to 0.001-1 s. The mechanism is a third-body interaction that detaches the donor, leaving an isolated, small period neutron star behind. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/FC1A2303A674483D1C080B5317D174DE/S174392131900005Xa.pdf/div-class-title-evolution-of-high-mass-x-ray-binaries-in-the-small-magellanic-cloud-div.pdf |
| Ending Page | 357 |
| Page Count | 5 |
| Starting Page | 353 |
| ISSN | 17439213 |
| e-ISSN | 17439221 |
| DOI | 10.1017/s174392131900005x |
| Journal | Proceedings of the International Astronomical Union |
| Issue Number | S346 |
| Volume Number | 14 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2018-08-01 |
| Access Restriction | Open |
| Subject Keyword | Proceedings of the International Astronomical Union Astronomy and Astrophysics Nuclear Physics General Neutron Evolution rays Accretion Disks |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
