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The L155NE Molecular OutflowEvidence 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.
Document ID
20210003901
Acquisition Source
Jet Propulsion Laboratory
Document Type
Other
External Source(s)
hdl:2014/29314
Authors
Wannier, P.G.
Butner, H.M.
Moriarty-Schieven, G.H.
Date Acquired
January 1, 1995
Publication Date
January 1, 1995
Publication Information
Publisher: UNKNOWN
Distribution Limits
Public
Copyright
Other
Technical Review
Keywords
protostar
nebula
outflow
Taurus

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