Published January 1997 | Version v1
Journal article

Microwave Spectra of Molecules of Astrophysical Interest. XXIV. Methanol (CH3OH and 13CH3OH)

  • 1. Department of Physical Sciences, University of New Brunswick, Saint John, New Brunswick, E2L 4L5 (CANADA)
  • 2. Optical Technology Division, National Institute of Standards and Technology, Gaithersburg, Maryland 20899 (United States)

Description

The available microwave and millimeter-wave spectra of methanol, CH3OH, and its most abundant isotopomer, 13CH3OH, are critically reviewed and supplemented with spectral frequency calculations derived from rotation-internal rotation analyses. For both species, global analyses of the torsional ground state, νt=0, and the first excited torsional state, νt=1, have been carried out in which all observed spectral lines are reproduced to within their measurement uncertainties. References are given for all data included. The primary objective of this review is to provide radio astronomers with complete spectral coverage of rotational transitions from 500 MHz to 1 THz, including the lower state energy and line strength for each transition, over the range in rotational quantum number J from 0 to 26. copyright 1997 American Institute of Physics and American Chemical Society.Key words: Internal rotation (or torsion); interstellar molecule; isotopomer; line strength; methanol; microwave and millimeter-wave spectra; radio astronomy; rotational transitions. copyright 1997 American Institute of Physics and American Chemical Society

Additional details

Publishing Information

Journal Title
Journal of Physical and Chemical Reference Data
Journal Volume
26
Journal Issue
1
Journal Page Range
p. 17-156.
ISSN
0047-2689
CODEN
JPCRBU