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Physical state of interstellar atomsBrief survey of the physical conditions along the lines of sight to reddened and unreddened stars, as determined from Copernicus observation of interstellar lines between 95 and 300 nm. Differences in ionization structure and density between clouds and the local intercloud medium are discussed. Some new data for beta Centauri is used to supplement the previously available data.
Document ID
19740063606
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
York, D. G.
(Princeton University New Observatory, Princeton, N.J., United States)
Date Acquired
August 7, 2013
Publication Date
October 8, 1974
Subject Category
Space Sciences
Accession Number
74A46356
Funding Number(s)
CONTRACT_GRANT: NAS5-1810
Distribution Limits
Public
Copyright
Other

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