A second outflow from L1551/IRS 5?

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Emission Spectra, Interstellar Matter, Molecular Clouds, Stellar Evolution, Astronomical Spectroscopy, Molecular Gases

Scientific paper

The detection of previously unreported high-velocity emission in the L1551 moleculaar cloud is reported. This emission may represent high-velocity molecular gas deflected out of the IRS 5 outflow or may indeed represent another independent outflow whose origin is IRS 5 or L1551NE. This region is revealed to be far more complex than previously suspected.

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