On the evidence for methane in Orion KL - A search for the 4.6 gigahertz line

Details On the evidence for methane in Orion KL - A search for the 4.6 gigahertz line On the evidence for methane in Orion KL - A search for the 4.6 gigahertz line

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...290l..63w&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 290, March 15, 1985, p. L63, L64.

Astronomy and Astrophysics

Astronomy

6

Astronomical Spectroscopy, Interstellar Gas, Methane, Molecular Spectra, Orion Nebula, Radio Astronomy, Microwave Spectra, Millimeter Waves

Scientific paper

A sensitive search for the J = 11 E(2)-E(1) transition of interstellar methane (CH4) has resulted in a peak upper limit which is much less than the value reported by Fox and Jennings in 1978. When combined with the negative results reported by Elldér et al. in 1980, these data rule out the detection of CH4 in Orion KL previously claimed by Fox and Jennings.

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