NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
Radiofrequency recombination lines as diagnostics of the cool interstellar medium.Quantitative details are given of a new diagnostic technique for the carbon and hydrogen (H I) recombination lines. Theoretical results are presented for conditions expected in H I clouds, and are compared with available observations for Orion A and NGC 2024.
Document ID
19720030859
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/180852
Authors
Dupree, A. K. (Harvard College Observatory Cambridge, Mass., United States)
Date Acquired
August 6, 2013
Publication Date
December 15, 1971
Publication Information
Publication: Astrophysical Journal
Volume: 170
Subject Category
Space Sciences
Accession Number
72A14525
Funding Number(s)
CONTRACT_GRANT: NSF GP-6750
CONTRACT_GRANT: NGL-22-007-006
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.

Related Records

There are no records associated with this record.
No Preview Available