Figure 2 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 2.

Radio to UV (dereddened) spectra with broken power-law spectral fits (solid lines; see the text). The dashed lines indicate possible ranges of parameters. The horizontal bars denote the uncertainty on the spectral break frequency on each date.

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