Editing X-ray binary (section)

== Intermediate-mass X-ray binary ==
An '''intermediate-mass X-ray binary''' ('''IMXB''') is a binary star system where one of the components is a neutron star or a black hole. The other component is an intermediate-mass star.<ref name=":1">{{Cite journal |bibcode = 2000ApJ...530L..93T|title = Formation of Millisecond Pulsars with Heavy White Dwarf Companions:Extreme Mass Transfer on Subthermal Timescales|journal = The Astrophysical Journal|volume = 530|issue = 2|pages = L93–L96|last1 = Tauris|first1 = Thomas M|last2 = Van Den Heuvel|first2 = Edward P. J|last3 = Savonije|first3 = Gerrit J|year = 2000|doi = 10.1086/312496|pmid = 10655173|arxiv = astro-ph/0001013|s2cid = 17772120}}</ref><ref name=":0">{{Cite journal |arxiv = astro-ph/0107261|bibcode = 2002ApJ...565.1107P|title = Evolutionary Sequences for Low- and Intermediate-Mass X-Ray Binaries|journal = The Astrophysical Journal|volume = 565|issue = 2|pages = 1107|last1 = Podsiadlowski|first1 = Ph|last2 = Rappaport|first2 = S|last3 = Pfahl|first3 = E. D|year = 2002|doi = 10.1086/324686|s2cid = 16381236}}</ref> An intermediate-mass X-ray binary is the origin for Low-mass X-ray binary systems.