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- W104865266 abstract "The relationship between optical outflows, as represented by Herbig-Haro (HH) objects and HH-like jets, and their associated molecular outflows is not well known. While molecular outflows are in many instances poorly collimated, this may not be true of HH outflows and it is certainly not the case with jets. Here we examine, through direct imaging and spectroscopy, the optical flow in the region east of Cepheus A, a well known molecular outflow source. Our images reveal several previously unseen HH objects in this region linked together by a virtual ellipse of HH emission. The major axis of this ellipse points directly at what is thought to be the driving source of activity in this area and it is argued that the optical, shocked molecular hydrogen, and radio emission all derive from a poorly collimated wind from Cep A" @default.
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- W104865266 date "1993-11-01" @default.
- W104865266 modified "2023-09-23" @default.
- W104865266 title "Optical evidence for a poorly-collimated wind from Cepheus A." @default.
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