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Discovery and Evolution of the New Black Hole Candidate Swift J1539.2–6227 during its 2008 Outburst

  • Authors: H. A. Krimm, J. A. Tomsick, C. B. Markwardt, C. Brocksopp, F. Grisé, P. Kaaret, and P. Romano

Krimm et al. 2011 The Astrophysical Journal 735 104.

  • Provider: AAS Journals

Caption: Figure 4.

Fits to the inner disk radius. Top: R in parameter from the kdblur model. Bottom: R in derived from the normalization to the diskbb model, assuming mass = 10  M , D = 10 kpc, and cos (θ) = 0.1. The first two of these parameters are typical values for BH systems and the third one is based on our average fitted value. The vertical lines and letters are as defined in the caption to Figure 1. The horizontal line in the top plot shows the weighted mean.

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