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Detection of 2.6-millimeter radiation probably due to nitrogen sulfideResults are reported for observations of millimeter-wavelength radiation in Sgr B2 at two frequencies corresponding to the transitions between the J = 5/2 and J = 3/2 Lambda-doublet sublevels in the 2 Pi(1/2) state of nitrogen sulfide. Difficulties in making a positive identification of the source of this radiation are discussed which result from the apparently anomalous ratio of the hyperfine components. However, it is noted that observations of the d-state by Gottlieb et al. (1975) showing the hyperfine components more exactly in their optically thin ratio confirm that the observed radiation is due to nitrogen sulfide.
Document ID
19750062757
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kuiper, T. B. H.
Kakar, R. K.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Rodriguez Kuiper, E. N.
(California, University Los Angeles, Calif., United States)
Zuckerman, B.
Date Acquired
August 8, 2013
Publication Date
September 15, 1975
Publication Information
Publication: Astrophysical Journal
Volume: 200
Subject Category
Astrophysics
Accession Number
75A46829
Funding Number(s)
CONTRACT_GRANT: NAS7-100
CONTRACT_GRANT: NSF GP-26218
Distribution Limits
Public
Copyright
Other

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