Black Holes and Pulsar Binaries
| dc.creator | Sigurdsson, Steinn | |
| dc.date | 2003-03-13 | |
| dc.date.accessioned | 2026-07-07T02:07:56Z | |
| dc.date.available | 2026-07-07T02:07:56Z | |
| dc.description | Stellar mass black holes are formed in the field, and are observed in binaries. Population synthesis estimates for the formation of BH-PSR binaries suggest these may be observed, but with very large formal uncertainties in the formation rate. In globular clusters, exchanges and binary interactions present more channels for BH-PSR formation, while ejection through recoil can remove a large fraction of the initial black hole population. A BH-PSR system ought to be observed in the near future, most likely in a globular cluster. | |
| dc.description | 6 pages, 2 figures, pasp.sty. To appear in "Radio Pulsars" (ASP Conf. Ser.), eds M. Bailes, D. Nice, & S. Thorsett | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0303312 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0303312 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5861 | |
| dc.subject | Astrophysics | |
| dc.title | Black Holes and Pulsar Binaries | |
| dc.type | text |