Abstract
An upper limit of the column density of the C5 linear molecule in translucent interstellar clouds is estimated from high-resolution (R = 80000) and very high signal-to-noise ratio (∼1000) echelle spectra. It is 1012 cm-2 per E(B - V) = 1 (two orders of magnitude lower than that of C2).
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APA
Galazutdinov, G. A., Musaev, F. A., & Krełowski, J. (2001). On the detection of the linear C5 molecule in the interstellar medium. Monthly Notices of the Royal Astronomical Society, 325(4), 1332–1334. https://doi.org/10.1046/j.1365-8711.2001.04388.x
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