GX 339-4

GX 339-4
	; GX 339-4 (artist's concept)
Observation data; EpochJ2000EquinoxJ2000
Constellation	Ara
Right ascension	17 02 49.5
Declination	-48 47 23
Characteristics
Apparent magnitude(B)	16.3
Apparent magnitude(V)	15.5
Apparent magnitude(J)	15.9
Apparent magnitude(H)	15.4
Apparent magnitude(K)	15.0
Variable type	LMXB
Other designations
	V821 Ara, 4U 1658-48, 3A 1659-487, 1RXS J170248.5-484719, 2MASS 17024936-4847228
Database references
SIMBAD	data

GX 339-4is a moderately strong variable galacticlow-mass X-ray binary(LMXB) source^[1]^[2]andblack holecandidate 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.^[3]

AnI band light curvefor GX 339-4, platted assuming an orbital period of 0.7 days. Adapted from Cowleyet al.(2002)^[4]

During the outbursts GX 339-4 shows evolution of quasi-periodic oscillations (QPOs). In the rising phase the QPO frequency monotonically increase as theCENBOLpropagates 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 wellmodeled by the propagating and oscillating shockin the sub-Keplerian flow. The entire spectrum also fits very well usingtwo component advective flow solution.

A strong, variablerelativistic jet,emitting from radio to infrared wavelengths was observed by several studies.^[5]^[6]^[7]

References

^SIMBAD
^Bradt, H.V.D., and McClintock, J.E., Annu. Rev. Astron. Astrophys., 21, 13-66 (1983)
^Hynes, R. I.; Steeghs, D.; Casares, J.; Charles, P. A.; O'Brien, K. (February 2003). "Dynamical Evidence for a Black Hole in GX 339-4".The Astrophysical Journal.583(2, pp. L95–L98): L95–L98.arXiv:astro-ph/0301127.Bibcode:2003ApJ...583L..95H.doi:10.1086/368108.S2CID 16820881.
^Cowley, A. P.; Schmidtke, P. C.; Hutchings, J. B.; Crampton, David (March 2002)."Optical Observations of the Black Hole Candidate GX 339−4 (V821 Arae)".The Astronomical Journal.123(3): 1741–1749.doi:10.1086/339028.S2CID 119867410.Retrieved25 October2021.
^Corbel, S.; Nowak, M. A.; Fender, R. P.; Tzioumis, A. K.; Markoff, S. (March 2003). "Radio/X-ray correlation in the low/hard state of GX 339-4".Astronomy and Astrophysics.400(3): 1007–1012.arXiv:astro-ph/0301436.Bibcode:2003A&A...400.1007C.doi:10.1051/0004-6361:20030090.S2CID 40809381.
^Casella, P.; Maccarone, T. J.; O'Brien, K.; Fender, R. P.; Russell, D. M.; van der Klis, M.; Pe'Er, A.; Maitra, D.; Altamirano, D.; Belloni, T.; Kanbach, G.; Klein-Wolt, M.; Mason, E.; Soleri, P.; Stefanescu, A.; Wiersema, K.; Wijnands, R. (May 2010). "Fast infrared variability from a relativistic jet in GX 339-4".Monthly Notices of the Royal Astronomical Society: Letters.404(1, pp. L21–L25): L21–L25.arXiv:1002.1233.Bibcode:2010MNRAS.404L..21C.doi:10.1111/j.1745-3933.2010.00826.x.S2CID 41202016.
^Gandhi, P.; Blain, A. W.; Russell, D. M.; Casella, P.; Malzac, J.; Corbel, S.; D'Avanzo, P.; Lewis, F. W.; Markoff, S.; Cadolle Bel, M.; Goldoni, P.; Wachter, S.; Khangulyan, D.; Mainzer, A. (October 2011). "A Variable Mid-infrared Synchrotron Break Associated with the Compact Jet in GX 339-4".The Astrophysical Journal Letters.740(1, article id. L13, 7 pp): L13.arXiv:1109.4143.Bibcode:2011ApJ...740L..13G.doi:10.1088/2041-8205/740/1/l13.S2CID 118406325.

External links

http://iopscience.iop.org/1538-3881/123/3/1741:Optical Observations of the black hole candidate GX 339-4 Cowely et al.
http://www.universetoday.com/89102/big-ol-black-hole-jets/:Big Ol’ Black Hole Jets

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[1] SIMBAD

[2] Bradt, H.V.D., and McClintock, J.E., Annu. Rev. Astron. Astrophys., 21, 13-66 (1983)

[3] Hynes, R. I.; Steeghs, D.; Casares, J.; Charles, P. A.; O'Brien, K. (February 2003). "Dynamical Evidence for a Black Hole in GX 339-4".The Astrophysical Journal.583(2, pp. L95–L98): L95–L98.arXiv:astro-ph/0301127.Bibcode:2003ApJ...583L..95H.doi:10.1086/368108.S2CID 16820881.

[Cowley-4] Cowley, A. P.; Schmidtke, P. C.; Hutchings, J. B.; Crampton, David (March 2002)."Optical Observations of the Black Hole Candidate GX 339−4 (V821 Arae)".The Astronomical Journal.123(3): 1741–1749.doi:10.1086/339028.S2CID 119867410.Retrieved25 October2021.

[5] Corbel, S.; Nowak, M. A.; Fender, R. P.; Tzioumis, A. K.; Markoff, S. (March 2003). "Radio/X-ray correlation in the low/hard state of GX 339-4".Astronomy and Astrophysics.400(3): 1007–1012.arXiv:astro-ph/0301436.Bibcode:2003A&A...400.1007C.doi:10.1051/0004-6361:20030090.S2CID 40809381.

[6] Casella, P.; Maccarone, T. J.; O'Brien, K.; Fender, R. P.; Russell, D. M.; van der Klis, M.; Pe'Er, A.; Maitra, D.; Altamirano, D.; Belloni, T.; Kanbach, G.; Klein-Wolt, M.; Mason, E.; Soleri, P.; Stefanescu, A.; Wiersema, K.; Wijnands, R. (May 2010). "Fast infrared variability from a relativistic jet in GX 339-4".Monthly Notices of the Royal Astronomical Society: Letters.404(1, pp. L21–L25): L21–L25.arXiv:1002.1233.Bibcode:2010MNRAS.404L..21C.doi:10.1111/j.1745-3933.2010.00826.x.S2CID 41202016.

[7] Gandhi, P.; Blain, A. W.; Russell, D. M.; Casella, P.; Malzac, J.; Corbel, S.; D'Avanzo, P.; Lewis, F. W.; Markoff, S.; Cadolle Bel, M.; Goldoni, P.; Wachter, S.; Khangulyan, D.; Mainzer, A. (October 2011). "A Variable Mid-infrared Synchrotron Break Associated with the Compact Jet in GX 339-4".The Astrophysical Journal Letters.740(1, article id. L13, 7 pp): L13.arXiv:1109.4143.Bibcode:2011ApJ...740L..13G.doi:10.1088/2041-8205/740/1/l13.S2CID 118406325.

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