04302+2247

okay, what's interesting about this is, check out the zoomed in infrared image from Padgett et al. (Astronomical Journal, vol. 117, p. 1490,1999):

This zooms in by about a factor of 30 more than the upper image. The dark band in the middle is probably a flared disk from which planets are forming. Usually, outflows are directed perpendicular to this disk. But in the upper image, we see jet emission in a very different direction. What is going on here? Is the jet emission coming from a different source? Is a binary at the center causing precession of the jet into very different directions? We don't know. The jet actually wobbles a bit but on a small scale compared to the direction of the nebula points to.