Figure 2 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 2.

Chandra High Energy Grating (HEG; top), Medium Energy Grating (MEG; top), and Low Energy Grating (LEG; bottom) spectra of V745 Sco obtained between 15.8 and 17.4 days into the outburst. Data are shown as the total accumulated counts per spectral bin, where the bin sizes are 0.0025 and 0.005 Å for HEG and MEG, respectively, and 0.0125 Å for LEG. Identifications of prominent spectral lines are indicated.

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