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  2. X-ray binary - Wikipedia

    en.wikipedia.org/wiki/X-ray_binary

    A high-mass X-ray binary (HMXB) is a binary star system that is strong in X rays, and in which the normal stellar component is a massive star: usually an O or B star, a blue supergiant, or in some cases, a red supergiant or a Wolf–Rayet star. The compact, X-ray emitting, component is a neutron star or black hole. [1]

  3. 3XMM J004232.1+411314 - Wikipedia

    en.wikipedia.org/wiki/3XMM_J004232.1+411314

    3XMM J004232.1+411314 is a low-mass X-ray binary hosted in the galaxy M31. It is the most luminous source of hard X-rays in the Andromeda Galaxy. It is also the most luminous source known that shows dips in the X-ray light curve. [1] The compact object in this system has been unambiguously identified as a neutron star with a spin period of 3 ...

  4. GX 339-4 - Wikipedia

    en.wikipedia.org/wiki/GX_339-4

    GX 339-4 is a moderately strong variable galactic low-mass X-ray binary (LMXB) source [1] [2] and black hole candidate that flares from time to time. From spectroscopic measurements, the mass of the black-hole was found to be at least of 5.8 solar masses.

  5. Category:X-ray binaries - Wikipedia

    en.wikipedia.org/wiki/Category:X-ray_binaries

    Main page; Contents; Current events; Random article; About Wikipedia; Contact us; Pages for logged out editors learn more

  6. Hercules X-1 - Wikipedia

    en.wikipedia.org/wiki/Hercules_X-1

    Her X-1 is the prototype for the massive X-ray binaries although it falls on the borderline, ~2 M ☉, between high- and low-mass X-ray binaries. [2] 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. [3]

  7. Ultraluminous X-ray source - Wikipedia

    en.wikipedia.org/wiki/Ultraluminous_X-ray_source

    Holmberg II X-1: This famous ULX resides in a dwarf galaxy. Multiple observations with XMM have revealed the source in both a low/hard and high/soft state, suggesting that this source could be a scaled-up X-ray binary or accreting IMBH. M74: Possibly containing an intermediate-mass black hole, as observed by Chandra in 2005.

  8. GRS 1915+105 - Wikipedia

    en.wikipedia.org/wiki/GRS_1915+105

    GRS 1915+105 or V1487 Aquilae is an X-ray binary star system containing a main sequence star and a black hole.Transfer of material from the star to the black hole generates a relativistic jet, making this a microquasar system.

  9. Vela X-1 - Wikipedia

    en.wikipedia.org/wiki/Vela_X-1

    Vela X-1 is a pulsing, eclipsing high-mass X-ray binary (HMXB) system, associated with the Uhuru source 4U 0900-40 and the supergiant star HD 77581. The X-ray emission of the neutron star is caused by the capture and accretion of matter from the stellar wind of the supergiant companion. Vela X-1 is the prototypical detached HMXB. [4]