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- GX_339-4 abstract "GX 339-4 is a moderately strong variable galactic low-mass X-ray binary (LMXB) source and black-hole candidate that flares from time to time.During the outbursts GX 339-4 shows evolution of quasi-periodic oscillations (QPOs). In the rising phase the QPO frequency monotonically increase as the CENBOL propagates closer to the black hole and in the declining phase the QPO frequency monotonically decreases since the CENBOL recedes away from the black hole after viscosity is decreased. The frequency variation is thus well modeled by the propagating and oscillating shock in the sub-Keplerian flow. The entire spectrum also fits very well using two component advective flow solution.".
- GX_339-4 thumbnail Flaring_Black_Hole.jpg?width=300.
- GX_339-4 wikiPageExternalLink 1995ApJ...455..623C.
- GX_339-4 wikiPageExternalLink 2012A%26A...542A..56N.
- GX_339-4 wikiPageExternalLink 1741:.
- GX_339-4 wikiPageExternalLink :.
- GX_339-4 wikiPageID "20188462".
- GX_339-4 wikiPageRevisionID "602095139".
- GX_339-4 appmag "15".
- GX_339-4 appmag "15.4".
- GX_339-4 appmag "15.5".
- GX_339-4 appmag "15.9".
- GX_339-4 appmag "16.3".
- GX_339-4 appmag1Passband "B".
- GX_339-4 appmag2Passband "V".
- GX_339-4 appmag3Passband "J".
- GX_339-4 appmag4Passband "H".
- GX_339-4 appmag5Passband "K".
- GX_339-4 constell "Ara".
- GX_339-4 dec "-484723".
- GX_339-4 epoch "J2000".
- GX_339-4 equinox "J2000".
- GX_339-4 hasPhotoCollection GX_339-4.
- GX_339-4 ra "170249.5".
- GX_339-4 variable "LMXB".
- GX_339-4 subject Category:Ara_(constellation).
- GX_339-4 subject Category:Objects_named_with_variable_star_designations.
- GX_339-4 subject Category:X-ray_binaries.
- GX_339-4 type CelestialBody.
- GX_339-4 type Star.
- GX_339-4 type PhysicalBody.
- GX_339-4 comment "GX 339-4 is a moderately strong variable galactic low-mass X-ray binary (LMXB) source and black-hole candidate that flares from time to time.During the outbursts GX 339-4 shows evolution of quasi-periodic oscillations (QPOs). In the rising phase the QPO frequency monotonically increase as the CENBOL propagates closer to the black hole and in the declining phase the QPO frequency monotonically decreases since the CENBOL recedes away from the black hole after viscosity is decreased.".
- GX_339-4 label "GX 339-4".
- GX_339-4 label "GX 339-4".
- GX_339-4 label "GX 339-4".
- GX_339-4 sameAs GX_339-4.
- GX_339-4 sameAs GX_339-4.
- GX_339-4 sameAs m.04yh9dp.
- GX_339-4 sameAs Q3084683.
- GX_339-4 sameAs Q3084683.
- GX_339-4 wasDerivedFrom GX_339-4?oldid=602095139.
- GX_339-4 depiction Flaring_Black_Hole.jpg.
- GX_339-4 isPrimaryTopicOf GX_339-4.
- GX_339-4 name "GX 339-4".
