High-velocity molecular jets

Journal Article · Sat Sep 01 04:00:00 EDT 1984 · Astrophys. J.; (United States)

DOI:https://doi.org/10.1086/162397· OSTI ID:6150744

Snell, R L; Scoville, N Z; Sanders, D B; Erickson, N R

The high-velocity CO emission in NGC 2071, GL 490, S140, and Orion have been mapped at 23'' or 48'' resolution. The outflow in NGC 2071 was clearly resolved in to two highly collimated opposing jets. The outflows in GL 490 and Orion do not appear as collimated, but are clearly bipolar. Only S140 shows no strong evidence of bipolar outflow.

• Research Organization: Five College Radio Astronomy Observatory, University of Massachusetts, Amherst
• OSTI ID: 6150744
• Journal Information: Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 284:1; ISSN ASJOA
• Country of Publication: United States
• Language: English

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