On the detection of the linear C5 molecule in the interstellar medium

Details On the detection of the linear C5 molecule in the interstellar medium On the detection of the linear C5 molecule in the interstellar medium

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001mnras.325.1332g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 325, Issue 4, pp. 1332-1334.

Astronomy and Astrophysics

Astronomy

5

Ism: Clouds, Ism: Molecules

Scientific paper

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 1012cm-2 per E(B-V)=1 (two
orders of magnitude lower than that of C2).

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