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Circumstellar CO Emission in S Stars I. Mass-Loss with Little or No Dust47 S stars have been searched for circumstellar CO (J=1-0 and/or 2-1) emission, and 29 have been detected, including 4 which show no evidence of dust in their IRAS LRS spectra and one with possibly no Tc (and therefore not an AGB star).
Document ID
20060042336
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/34560
Authors
Sahai, R.
Liechti, S.
Date Acquired
August 23, 2013
Publication Date
January 1, 1994
Publication Information
Publication: Astronomy and Astrophysics
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
late-type - radio lines: molecular - line: profiles
stars: mass-loss - stars: AGB and post-AGB Circumstellar matter - stars:

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