LABORATORY DETECTION OF A MOLECULAR BAND COINCIDENT WITH THE DIFFUSE INTERSTELLAR BAND AT $\lambda 4428$

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2000

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Ohio State University

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A strong molecular absorption band at 4429.27±0.04 {\AA}, closely centered on the strongest diffuse interstellar band at 4428.9±1.4 {\AA}, has been found in a supersonic molecular beam among the products of a discharge through benzene and other hydrocarbons. This agreement in wavelength to a few parts in 104 strongly suggests a common carrier. The width of the laboratory band is significantly less than that of the interstellar band, but this difference may be the result of the very low rotational temperature in the supersonic beam relative to that of a weakly polar molecule in the diffuse interstellar gas (100-200 K). Deuterium substitution suggests a carrier with elemental formula CxH5, where 3≤x≤6. Several candidate carriers are discussed.

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Author Institution: Harvard-Smithsonian Center faor Astrophysics, Division of Engineering and Applied Sciences, Harvard University

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