molecules:ism:si2c

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molecules:ism:si2c [2019/02/25 22:38] – external edit 127.0.0.1molecules:ism:si2c [2019/10/21 17:41] (current) – mueller
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 J. Cernicharo, M. C. McCarthy, C. A. Gottlieb, M. Agúndez, L. Velilla-Prieto, J. H. Baraban, P. B. Changala, M. Guélin, C. Kahane, M. A. Martin-Drumel, N. A. Patel, N. J. Reilly, J. F. Stanton, G. Quintana-Lacaci, S. Thorwirth, and K. H. Young,\\ J. Cernicharo, M. C. McCarthy, C. A. Gottlieb, M. Agúndez, L. Velilla-Prieto, J. H. Baraban, P. B. Changala, M. Guélin, C. Kahane, M. A. Martin-Drumel, N. A. Patel, N. J. Reilly, J. F. Stanton, G. Quintana-Lacaci, S. Thorwirth, and K. H. Young,\\
 reported on the\\ reported on the\\
-**[[http://dx.doi.org/10.1088/2041-8205/806/1/L3|Discovery of SiCSi in IRC+10216: A Missing Link between Gas and Dust Carriers of Si–C Bonds]]**\\+**[[https://doi.org/10.1088/2041-8205/806/1/L3|Discovery of SiCSi in IRC+10216: A Missing Link between Gas and Dust Carriers of Si–C Bonds]]**\\
 //Astrophys. J.// **806**, Art. No. L3 (2015).\\ //Astrophys. J.// **806**, Art. No. L3 (2015).\\
 More than hundred lines between 82 and 351 GHz were detected toward CW Leonis with the IRAM 30 m telescope. More than hundred lines between 82 and 351 GHz were detected toward CW Leonis with the IRAM 30 m telescope.
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