NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The millimeter and submillimeter rotational spectrum of the MgCN radical (X (sup 2) Sigma(+))The pure rotational spectrum of the MgCN radical has been recorded in the laboratory using millimeter/submillimeter direct absorption spectroscopy. Twenty-seven rotational transitions of the species were observed in the range 101-376 GHz and indicate that the molecule is linear with a (sup 2)Sigma(+) ground electronic state, as predicted by theory. Spin rotation interactions were resolved in the spectra, but no hyperfine splittings were observed, which would originate with the nitrogen nuclear spin. The rotational and fine-structure constants were determined for this radical from a nonlinear least-squares fit to the data using a (sup 2)Sigma Hamiltonian. MgCN is of astrophysical interest because it is the metastable isomer of MgNC, which recently has been detected toward IRC +10216
Document ID
19950029689
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Anderson, M. A.
(Arizona State Univ. Tempe, AZ, United States)
Steimle, T. C.
(Arizona State Univ. Tempe, AZ, United States)
Ziurys, L. M.
(Arizona State Univ. Tempe, AZ, United States)
Date Acquired
August 16, 2013
Publication Date
July 1, 1994
Publication Information
Publication: The Astrophysical Journal
Volume: 429
Issue: 1 pt
ISSN: 0004-637X
Subject Category
Astronomy
Accession Number
95A61288
Funding Number(s)
CONTRACT_GRANT: NAGW-2989
CONTRACT_GRANT: NSF AST-92-53682
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available