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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 8.

Plasma temperature vs. time for the V745 Sco blast wave estimated from Swift XRT data (see Section 4.4), together with that estimated from the NuSTAR observation by Orio et al. (2015). The electron temperature evolution of three of our analytical blast wave models, together with the expected temperature evolution based on the Sedov relations (see the text), is also shown.

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