Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...334..196c&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 334, Nov. 1, 1988, p. 196-208. NASA-supported research.
Astronomy and Astrophysics
Astrophysics
87
Carbon Monoxide, Interstellar Matter, Line Spectra, Molecular Flow, Collimation, Flow Geometry, Flow Velocity, Stellar Winds
Scientific paper
The RNO 43 and B335 molecular outflow regions both show a complex high-velocity emission pattern, previously attributed to several independent outflows. The authors present new CO and CS line observations which demonstrate that RNO 43 and B335 are in fact single highly collimated bipolar flows oriented nearly in the plane of the sky. The authors estimate the view angle between the line of sight and the flow axis to be 85° in RNO 43 and 82° in B335. They also study in detail the dynamics, the collimation, and the large-scale structure of the high-velocity lobes.
Cabrit Sylvie
Goldsmith Paul F.
Snell Ronald L.
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