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Her X-1 : ウィキペディア英語版
Hercules X-1

Hercules X-1 (Her X-1), also known as 4U1656+35, is a moderately strong X-ray binary source first studied by the Uhuru satellite.
It is composed of a neutron star accreting matter from a normal star (HZ Her) probably due to Roche lobe overflow.
==Intermediate-mass X-ray binary (IMXB)==

Her X-1 is the prototype for the massive X-ray binaries although it falls on the borderline, , between high- and low-mass X-ray binaries.〔
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.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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