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Observations of neutral atoms in the Rho Ophiuchi cloudNew observations of lines from neutral atoms in the lines of sight to three stars in the Rho Oph cloud are combined with literature data to look for evidence of density-enhanced regions with higher elemental depletions than those characterizing the cloud as a whole. The depletions inferred from neutral species, however, are comparable to those measured directly from observations of ions, suggesting that no strong density enhancements exist in the observed lines of sight. This conclusion is supported by electron densities derived from the observed ionization fractions, which also show no evidence for a strong variation of density with depth in the cloud. It appears that the overall density (and overall level of depletion) in the cloud is higher than in typical diffuse clouds, despite the apparent lack of strong condensations with enhanced relative depletions.
Document ID
19860050129
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Snow, T. P.
(Colorado Univ. Boulder, CO, United States)
Joseph, C. L.
(Colorado, University Boulder, United States)
Meyer, D. M.
(California, University Los Angeles, United States)
Date Acquired
August 12, 2013
Publication Date
April 1, 1986
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 303
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
86A34867
Funding Number(s)
CONTRACT_GRANT: NSG-7626
CONTRACT_GRANT: NSF AST-82-14989
Distribution Limits
Public
Copyright
Other

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