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Fig. 4.
CO(1–0) emission spectrum toward the GO248 galaxy center. The zero of the velocity scale (z = 0.05151) is centered at the peak of the low resolution H I 21 cm absorption line (Gupta et al. 2018a). The systemic velocity of the two merging galaxies G1 and G2 are indicated. The vertical scale is in mJy beam−1.
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