molecules:ism:ethylformiat

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molecules:ism:ethylformiat [2019/04/24 16:15] – muellermolecules:ism:ethylformiat [2026/03/04 11:34] (current) – mueller
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 In the group of the complex molecules detected by radio astronomical means, ethyl formate, C<sub>2</sub>H<sub>5</sub>OCHO, and //n//-propyl cyanide are among the largest. They have been detected in the famous massive star-forming region Sagittarius B2(N) in the course of a molecular line survey in the 3 mm frequency domain with additional observations at 2 and 1 mm carried out with the IRAM 30 m radio telescope.\\ In the group of the complex molecules detected by radio astronomical means, ethyl formate, C<sub>2</sub>H<sub>5</sub>OCHO, and //n//-propyl cyanide are among the largest. They have been detected in the famous massive star-forming region Sagittarius B2(N) in the course of a molecular line survey in the 3 mm frequency domain with additional observations at 2 and 1 mm carried out with the IRAM 30 m radio telescope.\\
 [[molecules:ism:aan|Aminoacetonitrile]] was detected earlier in the course of this molecular line survey.\\ [[molecules:ism:aan|Aminoacetonitrile]] was detected earlier in the course of this molecular line survey.\\
-At a rotational temperature of about 100 K, very many transitions of ethyl formate have non-negligible intensities. However, many of them are blended severely with emissions or absorptions of other molecules. Nevertheless, a considerable number of transitions of the lower energy //anti//-conformer are not or only slightly blended. Its column density in Sgr B2(N) is similar to that of formic acid, and about a factor of 15 lower than that of methyl formate.+At a rotational temperature of about 100 K, very many transitions of ethyl formate have non-negligible intensities. However, many of them are blended severely with emissions or absorptions of other molecules. Nevertheless, a considerable number of transitions of the lower energy //anti//-conformer are not or only slightly blended. Its column density in Sgr B2(N) is similar to that of formic acid, and about a factor of 15 lower than that of methyl formate.\\ 
 +\\
  
 The molecule was recently also identified in the Orion KL compact ridge region in the course of a molecular line survey carried out with the IRAM 30 m radio telescope.\\ The molecule was recently also identified in the Orion KL compact ridge region in the course of a molecular line survey carried out with the IRAM 30 m radio telescope.\\
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 **[[https://doi.org/10.1088/2041-8205/770/1/L13|Discovery of Methyl Acetate and Gauche Ethyl Formate in Orion]]**\\ **[[https://doi.org/10.1088/2041-8205/770/1/L13|Discovery of Methyl Acetate and Gauche Ethyl Formate in Orion]]**\\
 //Astrophys. J.// **770**, (2013) Art. No. L13.\\ //Astrophys. J.// **770**, (2013) Art. No. L13.\\
-Both conformers, //anti// and //gauche//, had about similar column densities, compatible with a kinetic temperature of 135 K. This agrees essentially with 150 K derived as rotational temperature of methyl acetate, which has a five times higher column density in this source than ethyl formate.+Both conformers, //anti// and //gauche//, had about similar column densities, compatible with a kinetic temperature of 135 K. This agrees essentially with 150 K derived as rotational temperature of methyl acetate, which has a five times higher column density in this source than ethyl formate.\\
  
-Ethyl formate is the second ester and the second formate to be detected in the ISM after [[molecules:ism:methylformiat|methyl formate]]. The isomeric [[molecules:ism:meac|methyl acetate]] was also detected very recently.+Ethyl formate is the second ester and the second formate to be detected in the ISM after [[molecules:ism:methylformiat|methyl formate]]. The isomeric [[molecules:ism:meac|methyl acetate]] was also detected very recently.\\ 
 +\\
  
 +In their work on\\
 +**[[https://doi.org/10.1051/0004-6361/202558316|Expanding the C3H6O2 Isomeric Interstellar Inventory: Discovery of Lactaldehyde and Methoxyacetaldehyde in G+0.693−0.027]]**\\
 +//Astron. Astrophys.// **706**, (2026) Art. No. A316.\\
 +M. Sanz-Novo, V. M. Rivilla, I. Jiménez-Serra, L. Colzi, S. Zeng, A. Megías, D. San Andrés, Á. López-Gallifa, A. Martínez-Henares, Z. T. P. Fried, B. A. McGuire, S. Martín, M. A. Requena-Torres, B. Tercero, P. de Vicente, L. Kolesniková, E. R. Alonso, E. J. Cocinero, J. C. Guillemin, and I. Kleiner\\
 +also report the detection of the anti conformer of ethyl formate in the course of a molecular line survey of this cold, shocked molecular cloud near Sagittarius B2 and in the Galactic center region. The number of unblended or slightly blended lines between 31 and 50 GHz is somewhat small, such that the identification should be viewed with some caution. The authors provide column density raios of the C<sub>3</sub>H<sub>6</sub>O<sub>2</sub> isomers.\\
 +\\
  
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-Contributor(s): H. S. P. Müller; 04, 2009; 07, 2013+Contributor(s): H. S. P. Müller; 04, 2009; 07, 2013; 03, 2026
  
  
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