Figure 3 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 3.

Best-fit three-temperature model (see the text) compared with the HEG (top) and MEG (middle) spectra binned by 10 pixels, and similar best-fit LEG spectrum (bottom) model and data binned by 5 pixels. The lower subpanels of each illustrate the fit residuals.

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