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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:\\ | 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,\\ | C. M. Walmsley, R. Bachiller, G. Pineau des Forêts, and P. Schilke,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
Since this is the only transition identified positively the detection is viewed as tentative in that paper. | 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: | More recently, the spatial distribution of this transition has been investigated: | ||
R. S. Furuya, C. M. Walmsley, K. Nakanishi, P. Schilke, and R. Bachiller, | R. S. Furuya, C. M. Walmsley, K. Nakanishi, P. Schilke, and R. Bachiller, | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
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Contributor(s): | Contributor(s): | ||
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