Show pageOld revisionsBacklinksBack to top This page is read only. You can view the source, but not change it. Ask your administrator if you think this is wrong. ===== On the Detection of Benzene in Extragalactic Sources ===== J. Bernard-Salas, E. Peeters, G. C. Sloan, J. Cami, S. Guiles, and J. R. Houck\\ obtained\\ **[[http://dx.doi.org/10.1086/509777|The //Spitzer// IRS spectrum of SMP LMC 11]]**\\ //Astrophys. J.// **652**, (2006) L29.\\ The spectrum resembles that of the protoplanetary nebula V353 Aur, which is somewhat better known as CRL (or AFGL) 618. As in the Galactic source, benzene was detected in absorption by its //ν//<sub>4</sub> band at 674.0 cm<sup>–1</sup> (or 14.84 μm). ---- Contributor(s): H. S. P. Müller; 5, 2012 ---- molecules/extragalactic/benzol_extragalactic.txt Last modified: 2019/02/25 22:38by 127.0.0.1