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Identification of RNO 43 and B335 as two highly collimated bipolar flows oriented nearly in the plane of the skyAn analysis of CO and CS line observations shows that RNO 43 and B335 are single highly collimated bipolar flows oriented nearly in the plane of the sky. The angle between the line of sight and the flow axis is estimated to be 85 deg in RNO 43 and 82 deg in B335. The results indicate that each of these flows must have a significant expansion velocity perpendicular to its axis, and that the flow in B335 must be driven by a mostly nonmolecular wind component.
Document ID
19890028072
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Cabrit, Sylvie
(Massachusetts, University Amherst; CNRS, Institut d'Astrophysique; Ecole Normale Superieure, Paris, France)
Goldsmith, Paul F.
(Massachusetts Univ. Amherst, MA, United States)
Snell, Ronald L.
(Massachusetts, University; Five College Radio Astronomy Observatory, Amherst, United States)
Date Acquired
August 14, 2013
Publication Date
November 1, 1988
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 334
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
89A15443
Funding Number(s)
CONTRACT_GRANT: NSF AST-85-12903
Distribution Limits
Public
Copyright
Other

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