Laboratory millimeter- and submillimeter-wave spectrum of C-13 methanol

Journal Article · Sat Aug 01 04:00:00 EDT 1987 · Astrophys. J., Suppl. Ser.; (United States)

DOI:https://doi.org/10.1086/191214· OSTI ID:5949200

Anderson, T; Herbst, E; De Lucia, F C

A comprehensive millimeter- and submillimeter-wave study of the rotational spectrum of (C-13)H/sub 3/OH is presented. Approximately 300 new transitions of this species were measured at frequencies up to 650 GHz, and the transitions were analyzed along with previously measured spectra using the internal axis method of Herbst et al. (1984). The resulting spectral constants allow prediction of an additional large number of transitions which should allow astronomers to identify many strong rotational lines of C-13 methanol throughout much of the submillimeter region. 23 references.

• Research Organization: Duke Univ., Durham, NC
• OSTI ID: 5949200
• Journal Information: Astrophys. J., Suppl. Ser.; (United States), Journal Name: Astrophys. J., Suppl. Ser.; (United States) Vol. 64; ISSN APJSA
• Country of Publication: United States
• Language: English

Related Subjects

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640301* -- Atomic
Molecular & Chemical Physics-- Beams & their Reactions
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ALCOHOLS
CARBON 13
CARBON ISOTOPES
CHEMICAL COMPOSITION
CHEMISTRY
COSMOCHEMISTRY
ELECTROMAGNETIC RADIATION
EVEN-ODD NUCLEI
HYDROXY COMPOUNDS
INTERSTELLAR SPACE
ISOTOPES
LIGHT NUCLEI
METHANOL
NUCLEI
ORGANIC COMPOUNDS
RADIATIONS
RADIOWAVE RADIATION
SPACE
SPECTRA
STABLE ISOTOPES