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| molecules:ism:formamid [2019/07/26 18:56] – mueller | molecules:ism:formamid [2019/10/23 22:03] (current) – mueller |
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| Formamide, HC(O)NH<sub>2</sub>, is a fairly typical hot core molecule that is quite abundant. The first transition of this molecule was detected toward Sgr B2 and likely toward Sgr A by\\ | Formamide, HC(O)NH<sub>2</sub>, is a fairly typical hot core molecule that is quite abundant. The first transition of this molecule was detected toward Sgr B2 and likely toward Sgr A by\\ |
| R. H. Rubin, G. W. Swenson, Jr., R. C. Solomon, and H. L. Flygare,\\ | R. H. Rubin, G. W. Swenson, Jr., R. C. Solomon, and H. L. Flygare,\\ |
| **[[http://cdsads.u-strasbg.fr/abs/1971ApJ...169L..39R|Microwave Detection of Interstellar Formamide]]**\\ | **[[https://ui.adsabs.harvard.edu/abs/1971ApJ...169L..39R|Microwave Detection of Interstellar Formamide]]**\\ |
| //Astrophys. J.// **169**, L39–L43 (1971).\\ | //Astrophys. J.// **169**, L39–L43 (1971).\\ |
| They detected all three Δ//F// = 0 hyperfine components of the //K<sub>a</sub>// = 1, //J// = 2 – 2 transition near 4619 MHz. Only the strongest component, overlapped in part with the H112α transition, was tentatively detected toward Sgr A.\\ | They detected all three Δ//F// = 0 hyperfine components of the //K<sub>a</sub>// = 1, //J// = 2 – 2 transition near 4619 MHz. Only the strongest component, overlapped in part with the H112α transition, was tentatively detected toward Sgr A.\\ |
| The detection of a second, related, 1 – 1 transition toward Sgr B2 and Sgr A was reported by\\ | The detection of a second, related, 1 – 1 transition toward Sgr B2 and Sgr A was reported by\\ |
| C. A. Gottlieb, P. Palmer, L. J. Richard, and B. Zuckerman\\ | C. A. Gottlieb, P. Palmer, L. J. Richard, and B. Zuckerman\\ |
| **[[http://cdsads.u-strasbg.fr/abs/1973ApJ...182..699G|Studies of Interstellar Formamide]]**\\ | **[[https://ui.adsabs.harvard.edu/abs/1973ApJ...182..699G|Studies of Interstellar Formamide]]**\\ |
| //Astrophys. J.// **182**, 699–710 (1973). | //Astrophys. J.// **182**, 699–710 (1973). |
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| Contributor(s): H. S. P. Müller; 05, 2009; 08, 2012; 02, 2013; 06, 2016; 10, 2017; 01, 2019 | Contributor(s): H. S. P. Müller; 05, 2009; 08, 2012; 02, 2013; 06, 2016; 10, 2017; 01, 2019 |
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