Formation of Low-Mass X-ray Binaries. III. A New Formation Mechanism: Direct Supernova

Vassiliki Kalogera

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Formation of Low-Mass X-ray Binaries. III. A New Formation Mechanism: Direct Supernova

Vassiliki Kalogera

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Abstract

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.

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Vassiliki Kalogera. 1996-08-11. Formation of Low-Mass X-ray Binaries. III. A New Formation Mechanism: Direct Supernova. https://arxiv.org/abs/astro-ph/9608058

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