Ultra-compact X-ray binaries with high luminosity: a key for a new scenario

Abstract

Abstract Ultra-compact X-ray binaries (UCXBs) are accreting systems with periods less than 1 hour, which qualifies them to contain a degenerate donor-companion. One would expect such systems to have the easiest theoretical explanation, compared to other kinds of X-ray binaries. Nonetheless, current theory fails to explain high mass transfer (MT) rates in three recently well observed long-period UCXBs. We find that this range of MT rates can be maintained if the donor is a remnant of an out-of-thermal-equilibrium naked core of a giant which was revealed in a very recent episode of a common envelope (CE) event.

Locations

• Proceedings of the International Astronomical Union - View - PDF
• arXiv (Cornell University) - View - PDF
• DataCite API - View