Formation of Low-Mass X-ray Binaries. III. A New Formation Mechanism: Direct Supernova
| dc.creator | Kalogera, Vassiliki | |
| dc.date | 1996-08-11 | |
| dc.date.accessioned | 2026-07-07T02:21:44Z | |
| dc.date.available | 2026-07-07T02:21:44Z | |
| dc.description | We propose a new formation mechanism (direct-supernova) for low-mass X-ray binaries (LMXBs) that does not involve any prior phase of mass transfer. Survival through the supernova (SN) explosion and shrinkage of the orbit is achieved by a kick velocity of appropriate magnitude and direction imparted to the neutron star at its birth. We present analytical population synthesis calculations of LMXBs forming via both the direct-SN and the helium-star SN mechanisms, and compare the results. We find that the direct-SN channel contributes a non-negligible fraction of the total LMXB population, depending strongly on the r.m.s. magnitude of the kick velocity. More importantly, the direct-SN mechanism provides a natural way for the formation of low-mass binary pulsars in nearly circular orbits with orbital periods in excess of about 100 days, which cannot have been formed via the helium-star SN mechanism. | |
| dc.description | 11 pages, 7 Postscript Figures, uses aaspp4.sty. Accepted for publication in the Astrophysical Journal | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9608058 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9608058 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10614 | |
| dc.subject | Astrophysics | |
| dc.title | Formation of Low-Mass X-ray Binaries. III. A New Formation Mechanism: Direct Supernova | |
| dc.type | text |