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Fig. 3

image

As Fig. 2, but showing three FLAMES-UVES spectra (MJD = 56645.57, 56645.57, 56697.69), and focussing on the N V λλ4604, 4620 and N III λλ4634, 4641 lines. Both components contribute to the N V λλ4604, 4620 lines, while the cooler secondary dominates the N IIIλλ4634, 4641 lines.

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