Fig. 27.
Kinematics of the two images A3 (blue) and A2 (red, reversed) in SDSS 1038+4849 derived from the Hα observations (stars) and from the [O IIIλ5007] observations (triangles). The resulting curves of A2 and A3 have the typical reversed U shape of interacting systems, suggesting that the A2 and A3 images are composed of at least three clumps that are interacting with each other.
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