Fig. 2
Chandra MEG ± 1 order X-ray spectrum between spin-phases φ67 = 0.9 and 1.1 (i.e., the range of phases where the observer has the most unextinguished view of the accretion column) fit with an XSPEC variable-abundance isobaric cooling flow model (vmcflow). The absorption column, NH, is smaller than 1020 cm-2, as expected, while the shock temperature is 
keV.
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