The L1551NE molecular outflow

Details The L1551NE molecular outflow The L1551NE molecular outflow

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...445l..55m&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 445, no. 1, p. L55-L58

Astronomy and Astrophysics

Astronomy

31

Infrared Astronomy, Interstellar Matter, Molecular Clouds, Molecular Flow, Protostars, Star Formation, Far Infrared Radiation, Nebulae, Stellar Luminosity

Scientific paper

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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