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Far-ultraviolet fluorescence of carbon monoxide in the red giant Arcturus. II - Analysis of high-dispersion IUE spectraFaint, diffuse emissions near 1380 A in deeply exposed IUE spectrograms of the red giant Arcturus very likely are associated with bands of the A-X fourth-positive system of carbon monoxide, fluoresced by multiplet UV2 of neutral oxygen near 1305 A. Numerical simulations indicate that the strength of the CO bands is exceedingly sensitive, in the best available one-dimensional model of the chromosphere of Arcturus, to a delicate balance between the rapid inward attenuation of the oxygen radiation field and the rapid outward decline of the molecular absorptivity. The fortuitous character of the overlap region in the single-component model argues that one should also consider the possibility that the pumping occurs in a highly inhomogeneous chromosphere, of the type proposed in previous studies of Arcturus based on observations of the infrared absorption bands of CO.
Document ID
19870029349
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ayres, T. R.
(Colorado, University Boulder, United States)
Date Acquired
August 13, 2013
Publication Date
September 1, 1986
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 308
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
87A16623
Funding Number(s)
CONTRACT_GRANT: NSF AST-85-07029
CONTRACT_GRANT: NGL-06-003-057
CONTRACT_GRANT: NAG5-199
CONTRACT_GRANT: NSF AST-82-03450
Distribution Limits
Public
Copyright
Other

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