molecules:extragalactic:l-c3h_extragalactic [CDMS classic documentation]

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===== On the Detection of Propynylidyne, l-C3H, in Extragalactic Sources =====

S. Muller, A. Beelen, M. Guélin, S. Aalto, J. H. Black, F. Combes, S. J. Curran, P. Theule, and S. N. Longmore\\
used the Australia Telescope Compact Array (ATCA) to study the molecular content of a foreground galaxy at //z// = 0.89 (FG0.89 consisting of two subsources, FG0.89SW and FG0.89NO) in absorption toward the quasar PKS 1830-211:\\
**[[https://doi.org/10.1051/0004-6361/201117096|Molecules at //z// = 0.89: A 4-mm-Rest-Frame Absorption-Line Survey toward PKS 1830-211]]**\\
//Astron. Astrophys.// **535**, (2011) Art. No. A103.\\
Propynylidyne, //l//-C<sub>3</sub>H, was identified by its //J// = 7/2 – 5/2 transition of the lower energy fine structure component <sup>2</sup>Π<sub>1/2</sub> with a rest frequency of 76.2 GHz. The Λ-doubling was marginally resolved, the H-hyperfine structure was not resolved. The detection can probably be viewed as secure because of the strong signal and the moderate line number density.


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Contributor(s): H. S. P. Müller; 5, 2012

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