(a) Three outflows are seen in close proximity: MHO 1633, MHO 1634, and MHO 1635. MHO 1633, seen in the upper left, is an asymmetric curved flow emerging from the point source J103648.0−583819. Beneath it lies MHO 1634, a bipolar outflow emerging from SPICY 7423 and the spectacular reflection nebula that surrounds it. H2 knots in MHO 1634 stand out prominently in the continuum-subtracted H2 image. Below MHO 1634 and with a nearly parallel outflow axis is MHO 1635. Curved emission seen immediately below the candidate driving source J103646.7−583805 suggests the lower part of the outflow is blueshifted. The upper portion of the outflow points towards another string of H2 knots that lies between MHO 1634 and MHO 1635, making it unclear to which flow they belong. (b) F200W–F335M image of the reflection nebula at the origin of MHO 1634. Some knots can be seen in the upper right, likely due to shocked H2 in the F200W filter. (c) F200W–F335M image of the origin of MHO 1635. Like MHO 1634, some knots are also visible.
