Fast infrared variability from a relativistic jet in GX 339--4


Casella, P., Maccarone, T. .J., O'Brien, K., Fender, R.P., Russell, D.M., van der Klis, M., Pe'er, A., Maitra, M., Altamirano, D., Belloni, T., Kanbach, G., Klien-Wolt, M., Mason, E., Soleri, P., Stefanescu, A., Wiersema, K. and Wijnands, R. (2009) Fast infrared variability from a relativistic jet in GX 339--4. Monthly Notices of the Royal Astronomical Society, 1-5.

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Description/Abstract

We present the discovery of fast infrared/X-ray correlated variability in the black-
hole transient GX 339-4. The source was observed with sub-second time resolution
simultaneously with VLT/ISAAC and RXTE/PCA in August 2008, during its persis-
tent low-
ux highly variable hard state. The data show a strong correlated variability,
with the infrared emission lagging the X-ray emission by 100 ms. The short time de-
lay and the nearly symmetric cross-correlation function, together with the measured
brightness temperature of 2:5 106 K, indicate that the bright and highly variable
infrared emission most likely comes from a jet near the black hole. Under standard
assumptions about jet physics, the measured time delay can provide us a lower limit
of

Item Type: Article
ISSNs: 0035-8711 (print)
Subjects: Q Science > QC Physics
Divisions: University Structure - Pre August 2011 > School of Physics and Astronomy > Astronomy and Space Science
Item ID: 69884
Date Deposited: 04 Jan 2010
Last Modified: 03 Jul 2012 15:16
Contributors: Casella, P. (Author)
Maccarone, T. .J. (Author)
O'Brien, K. (Author)
Fender, R.P. (Author)
Russell, D.M. (Author)
van der Klis, M. (Author)
Pe'er, A. (Author)
Maitra, M. (Author)
Altamirano, D. (Author)
Belloni, T. (Author)
Kanbach, G. (Author)
Klien-Wolt, M. (Author)
Mason, E. (Author)
Soleri, P. (Author)
Stefanescu, A. (Author)
Wiersema, K. (Author)
Wijnands, R. (Author)
Date: 8 December 2009
Status: Published
Contact Email Address: p.casella@soton.ac.uk
URI: http://eprints.soton.ac.uk/id/eprint/69884

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