molecules:ism:formic_acid

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molecules:ism:formic_acid [2019/10/23 17:06] – muellermolecules:ism:formic_acid [2019/10/23 17:09] (current) – mueller
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 Formic acid, HC(O)OH, seems to be a fairly typical hot core molecule that is quite abundant. The 1<sub>11</sub> – 1<sub>10</sub> transition of this molecule was the first one to be detected – toward the massive star-forming region Sgr B2 near the Galactic center:\\ Formic acid, HC(O)OH, seems to be a fairly typical hot core molecule that is quite abundant. The 1<sub>11</sub> – 1<sub>10</sub> transition of this molecule was the first one to be detected – toward the massive star-forming region Sgr B2 near the Galactic center:\\
 B. Zuckerman, J. A. Ball, and C. A. Gottlieb,\\ B. Zuckerman, J. A. Ball, and C. A. Gottlieb,\\
-**[[http://cdsads.u-strasbg.fr/doi/10.1086/180663|Microwave Detection of Interstellar Formic Acid]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1971ApJ...163L..41Z|Microwave Detection of Interstellar Formic Acid]]**\\
 //Astrophys. J.// **163**, L41–L45 (1971);\\ //Astrophys. J.// **163**, L41–L45 (1971);\\
 the detection of a second transition was reported by\\ the detection of a second transition was reported by\\
 G. Winnewisser and E. Churchwell,\\ G. Winnewisser and E. Churchwell,\\
-**[[http://adsabs.harvard.edu/doi/10.1086/181890|Detection of Formic Acid in Sagittarius B2 by its 2<sub>11</sub> – 2<sub>12</sub> Transition]]**\\+**[[https://ui.adsabs.harvard.edu/abs/1975ApJ...200L..33W|Detection of Formic Acid in Sagittarius B2 by its 2<sub>11</sub> – 2<sub>12</sub> Transition]]**\\
 //Astrophys. J.// **200**, L33–L36 (1975). //Astrophys. J.// **200**, L33–L36 (1975).
  
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