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Physical structure of the IRC+10216 wind: Molecular sidereoarcheologyWe present KAO observations of the CO J=9-8 and 12-11 lines in the C-star IRC+10216; these are the highest rotational transitions so far observed in any AGB star. A model is developed for the CO emission by IRC+10216 in all the observed CO rotational transitions.
Document ID
19960003673
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Skinner, C. J. (Lawrence Livermore National Lab. Livermore, CA., United States)
Justtanont, K. (NASA Ames Research Center Moffett Field, CA, United States)
Tielens, Alexander G. G. M. (NASA Ames Research Center Moffett Field, CA, United States)
Betz, A. L. (Colorado Univ. Boulder, CO., United States)
Boreiko, R. T. (Colorado Univ. Boulder, CO., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1995
Publication Information
Publication: Astronomical Society of the Pacific, Airborne Astronomy Symposium on the Galactic Ecosystem: From Gas to Stars to Dust, Volume 73
Subject Category
Astrophysics
Accession Number
96N13683
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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