molecules:extragalactic:hc3n_extragalactic

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molecules:extragalactic:hc3n_extragalactic [2019/02/25 22:38] – external edit 127.0.0.1molecules:extragalactic:hc3n_extragalactic [2019/10/22 16:23] (current) – mueller
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 R. Mauersberger, C. Henkel, and L. J. Sage,\\ R. Mauersberger, C. Henkel, and L. J. Sage,\\
-**[[http://adsabs.harvard.edu/abs/1990A%26A...236...63M|Dense gas in nearby galaxies. III – HC<sub>3</sub>N as an extragalactic density probe]]**,\\+**[[https://ui.adsabs.harvard.edu/abs/1990A%26A...236...63M|Dense gas in nearby galaxies. III – HC<sub>3</sub>N as an extragalactic density probe]]**,\\
 //Astron. Astrophys.// **236**, 63–68 (1990). //Astron. Astrophys.// **236**, 63–68 (1990).
  
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 A tentative detection of the //J// = 10 – 9 transition toward IC342 or M82 with the IRAM 30 m telescope had been reported previously:\\ A tentative detection of the //J// = 10 – 9 transition toward IC342 or M82 with the IRAM 30 m telescope had been reported previously:\\
 C. Henkel, R. Mauersberger, and P. Schilke,\\ C. Henkel, R. Mauersberger, and P. Schilke,\\
-**[[http://adsabs.harvard.edu/abs/1988A%26A...201L..23H|Molecules in external galaxies – The detection of CN, C<sub>2</sub>H, and HNC, and the tentative detection of HC<sub>3</sub>N]]**,\\+**[[https://ui.adsabs.harvard.edu/abs/1988A%26A...201L..23H|Molecules in external galaxies – The detection of CN, C<sub>2</sub>H, and HNC, and the tentative detection of HC<sub>3</sub>N]]**,\\
 //Astron. Astrophys.// **201**, L23–L26 (1988). //Astron. Astrophys.// **201**, L23–L26 (1988).
  
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 F. Costagliola and S. Aalto,\\ F. Costagliola and S. Aalto,\\
-**[[http://dx.doi.org/10.1051/0004-6361/200913370|Vibrationally Excited HC<sub>3</sub>N in NGC 4418]]**,\\+**[[https://doi.org/10.1051/0004-6361/200913370|Vibrationally Excited HC<sub>3</sub>N in NGC 4418]]**,\\
 //Astron. Astrophys.// **515**, Art. No. A71 (2010). //Astron. Astrophys.// **515**, Art. No. A71 (2010).
  
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 Contributor(s): S. Thorwirth; 09/2005; H. S. P. Müller, 07, 2010 Contributor(s): S. Thorwirth; 09/2005; H. S. P. Müller, 07, 2010
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