NASA NTRS · 19950056284
The L1551NE molecular outflow
Abstract
L1551NE is a very young protostar (class I or perhaps class 0), located very close to L1551NE IRS 5. It is the second brightest far-infrared source in the Taurus molecular cloud complex, but its proximity to the brightest source IRS 5 has prevented effective observations of any molecular outflow. We here present evidence that it does indeed process an outflow, that the optical/infrared reflection nebula is associated with the blueshifted outflow lobe, and that the L1551W outflow does not originate from L1551NE, as has been suggested.
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Moriarty-Schieven, G. H., Butner, H. M., Wannier, P. G.. 1995-05-20. The L1551NE molecular outflow. https://ntrs.nasa.gov/citations/19950056284
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