Figure 1 from An Evolving Compact Jet in the Black Hole X-Ray Binary MAXI J1836

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An Evolving Compact Jet in the Black Hole X-Ray Binary MAXI J1836–194

Authors: D. M. Russell, T. D. Russell, J. C. A. Miller-Jones, K. O'Brien, R. Soria, G. R. Sivakoff, T. Slaven-Blair, F. Lewis, S. Markoff, J. Homan, D. Altamirano, P. A. Curran, M. P. Rupen, T. M. Belloni, M. Cadolle Bel, P. Casella, S. Corbel, V. Dhawan, R. P. Fender, E. Gallo, P. Gandhi, S. Heinz, E. G. Körding, H. A. Krimm, D. Maitra, S. Migliari, R. A. Remillard, C. L. Sarazin, T. Shahbaz, and V. Tudose

Russell et al. 2013 The Astrophysical Journal Letters 768 L35.

Provider: AAS Journals

Caption: Figure 1.

Upper panel: radio, IR, optical, and UV light curves of the 2011 outburst of MAXI J1836−194. Where error bars are not visible they are smaller than the symbols. As well as VLT/VISIR mid-IR, FT optical, and Swift UVOT optical/UV data ( v band, b band, and the average flux of the three UV filters, w1, m2, and w2) we also include i′- and K _S-band fluxes on August 30 (MJD 55803) from Rau et al. (2011). Center panel: X-ray ( RXTE) light curve. Lower panel: X-ray color (two intensity ratios are given). The vertical dashed lines illustrate state transition dates (from Ferrigno et al. 2012).

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