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Please use this identifier to cite or link to this item:
http://hdl.handle.net/2014/29314
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| Title: | The L155NE Molecular Outflow |
| Authors: | Moriarty-Schieven, G.H.
Butner, H.M.
Wannier, P.G. |
| Issue Date: | 1995 |
| Citation: | The Astrophysical Journal |
| 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. |
| URI: | http://hdl.handle.net/2014/29314 |
| Appears in Collections: | JPL TRS 1992+
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