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--- molecules:ism:feo [2019/02/25 22:38] – external edit 127.0.0.1
+++ molecules:ism:feo [2019/10/18 13:00] (current) – mueller
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 FeO had been identified previously by its electronic spectrum in stellar atmospheres. Very recently, its lowest energy //J// = 5 – 4 transition has been detected in the ISM towards Sgr B2 M:\\
 C. M. Walmsley, R. Bachiller, G. Pineau des Forêts, and P. Schilke,\\
-**[[http://dx.doi.org/10.1086/339694|Detection of FeO toward Sagittarius B2]]**\\
+**[[https://doi.org/10.1086/339694|Detection of FeO toward Sagittarius B2]]**\\
 //Astrophys. J.// **566**, L109–L112 (2002).\\
 Since this is the only transition identified positively the detection is viewed as tentative in that paper.
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 More recently, the spatial distribution of this transition has been investigated:\\
 R. S. Furuya, C. M. Walmsley, K. Nakanishi, P. Schilke, and R. Bachiller,\\
-**[[http://dx.doi.org/10.1051/0004-6361:20031304|Interferometric observations of FeO towards Sagittarius B2]]**\\
+**[[https://doi.org/10.1051/0004-6361:20031304|Interferometric observations of FeO towards Sagittarius B2]]**\\
 //Astron. Astrophys.// **409**, L21–L24 (2003).
@@ Line 16: / Line 16: @@
 Contributor(s): H. S. P. Müller; 09, 2003
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