Fig. 1
Optical (BGR) overview of the star forming region centered on HH 250 IRS = IRAS 19190+1048. The red asterisk marks the embedded source, and two components of the HH 250 flow are marked (A is the brighter knot, B is the fainter one). The image is 5.′ 7 across, with north to the top and east to the left. Image courtesy Adam Block.
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