C.P. 6128, Succ. HgCdTe array with cold transfer optics yielding an image scale of 0.035. The wave front sensor of the AOB was centered on the nucleus except for He 2-10 where a 14.5 mag star located 20'' away from the galaxy was used for closing the loop. In the following we describe some of the results obtained on He 2-10.
East is left and north is up.
The faint sources to the east have . The near-infrared morphology of region B is more reminiscent of a tidal tail than a small companion. There is also a feature north-west of the nucleus which looks very much like a faint tidal tail. The authors argued that these globulars could have been formed as a result of a merger event. Thanks to the relatively large field of view of KIR, it was possible to get an accurate registration of both KIR and HST images.