NASA NTRS · 20210003901
The L155NE Molecular Outflow
Abstract
Evidence is presented that L1551NE, a very young protostar in the Taurus molecular cloud complex, possesses an outflow, that the optical/infrared reflection nebula is associated with the blue shifted outflow lobe, and that the L1551W outflow does not originate from L1551NE as has been suggested.
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Wannier, P.G., Butner, H.M., Moriarty-Schieven, G.H.. 1995-01-01. The L155NE Molecular Outflow. https://ntrs.nasa.gov/citations/20210003901
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