Sub-millimeter Spectroscopy of Astrophysically Interesting Metal-Containing Molecules

Details Sub-millimeter Spectroscopy of Astrophysically Interesting Metal-Containing Molecules Sub-millimeter Spectroscopy of Astrophysically Interesting Metal-Containing Molecules

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nla..work..168z&link_type=abstract

NASA Laboratory Astrophysics Workshop, held May 1-3 2002 at NASA Ames Research Center, Moffett Field, CA 94035-1000. Publisher:

Astronomy and Astrophysics

Astrophysics

Scientific paper

With the advent of SOFIA and Herschel, new spectral windows will be opened for spectroscopy in the sub- millimeter region. To conduct science in this band, laboratory measurements must be carried out to provide accurate transition frequencies for molecular identification and physical interpretation. We are presently con- ducting such measurements using gas-phase submm direct absorption techniques. Of particular interest are simple molecules containing iron-peak elements, including carbides, and metal hydride ions (MH+), both of which possess favorable transitions at submm wavelengths.

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