Abstract
We have observed the bipolar outflow source NGC 1333 (HH 7–11) in theJ=2–1 transition of12CO, and find evidence for a strong westerly termination of the red outflow lobe at a velocityV lsr ∼27 km s−1, together with maximal mean red-flow velocities Δv centred upon both the driving source SVS 13 and the westerly limit of the outflow zone. As a consequence, we propose a model for the source in which the red-shifted outflow is directly im**ing upon a nearby molecular cloud, causing extensive surface erosion and/or diversion of the jet material.
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Phillips, J.P., Mampaso, A. New insights into a familiar friend: COJ=2–1 map** of the bipolar outflow source NGC 1333 (HH 7–11). Astrophys Space Sci 171, 189–193 (1990). https://doi.org/10.1007/BF00646844
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DOI: https://doi.org/10.1007/BF00646844