Figure 1 from COLLIMATION AND ASYMMETRY OF THE HOT BLAST WAVE FROM THE RECURRENT NOVA V745 Sco

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COLLIMATION AND ASYMMETRY OF THE HOT BLAST WAVE FROM THE RECURRENT NOVA V745 Sco

Authors: Jeremy J. Drake, Laura Delgado, J. Martin Laming, Sumner Starrfield, Vinay Kashyap, Salvatore Orlando, Kim L. Page, M. Hernanz, J.-U. Ness, R. D. Gehrz, Daan van Rossum, and Charles E. Woodward

2016 The Astrophysical Journal 825 95.

Provider: AAS Journals

Caption: Figure 1.

Swift XRT count rate for V745 Sco as a function of the time since the outburst was first identified. The times of Chandra high-resolution spectroscopic observations are indicated by the shaded regions. The times of SSS onset and end discussed by Page et al. (2015) are also illustrated.

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