Figure 10.
MHO 1645 and its probable driving source, J103654.4−583618, lie ∼3 arcsec inside the edge of the cloud. The bipolar outflow propagates nearly parallel to the cloud edge. A second outflow, MHO 1646, appears to emerge from the same source with an orientation nearly perpendicular to MHO 1645.

MHO 1645 and its probable driving source, J103654.4−583618, lie ∼3 arcsec inside the edge of the cloud. The bipolar outflow propagates nearly parallel to the cloud edge. A second outflow, MHO 1646, appears to emerge from the same source with an orientation nearly perpendicular to MHO 1645.

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