MagAO-X/IFU data of the binary. Left panel: IFU images of the binary stacked along the wavelength channel. The image is not rotated to place North up. Middle panel: spectrum of star A and the first three principal components of star B’s spectra. The grey area shows the H_α line band. Star A presents H_α absorption. The first component presents H_α emission from star B. The third component (K=3) is the contamination from star A. Right panel: smoothed version of the middle panel by a Gaussian kernel with a standard deviation of 0.48 Å. The grey area shows the H_α line band.