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Crutcher on-camera: text

What we 've done is process the S106 data we obtained at Hat Creek with the supercomputers at NSCA. What we now have are three-dimensional images of this region of recent star formation. What we'd now like to do is to analyze these data in terms of the structure of the region, the kinematics, the motions of the gas, to try and understand the interactions between the gas and the newly-formed star.

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Copyright, (c) 1995: Board of Trustees, University of Illinois

NCSA. Last modified 11/13/95.