Evolution of Low- and Intermediate-Mass X-Ray Binaries

Details Evolution of Low- and Intermediate-Mass X-Ray Binaries Evolution of Low- and Intermediate-Mass X-Ray Binaries

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..289..273l&link_type=abstract

The Proceedings of the IAU 8th Asian-Pacific Regional Meeting, Volume I, held 2-5 July 2002 at National Center of Sciences, Hito

Astronomy and Astrophysics

Astronomy

1

Scientific paper

In the standard scenario, low-mass binary pulsars (LMBPs) are the descendants of low-mass X-ray binaries (LMXBs). More recent investigations indicate that a large fraction of the observed LMXBs may actually have started their lives as intermediate-mass X-ray binaries (IMXBs). In this paper we summarize the existing problems and progress in the evolutionary studies of LMXBs and IMXBs with respect to LMBP formation.

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