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molecules:ism:eme [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:eme [2022/01/18 12:35] (current) – mueller | ||
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===== On Ethyl Methyl Ether, C2H5OCH3, in the ISM ===== | ===== On Ethyl Methyl Ether, C2H5OCH3, in the ISM ===== | ||
- | G. W. Fuchs, U. Fuchs, T. F. Giesen, and F. Wyrowski,\\ | + | G. W. Fuchs, U. Fuchs, T. F. Giesen, and F. Wyrowski\\ |
- | **[[http://dx.doi.org/ | + | reported on\\ |
+ | **[[https:// | ||
A new Look at a Complex Molecule in Selected Hot Core Regions]]**\\ | A new Look at a Complex Molecule in Selected Hot Core Regions]]**\\ | ||
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
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P. B. Carroll, B. A. McGuire, G. A. Blake, A. J. Apponi, L. M. Ziurys, and A. Remijan,\\ | P. B. Carroll, B. A. McGuire, G. A. Blake, A. J. Apponi, L. M. Ziurys, and A. Remijan,\\ | ||
reported on\\ | reported on\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
A Rigorous Attempt to Confirm // | A Rigorous Attempt to Confirm // | ||
// | // | ||
Line 18: | Line 19: | ||
B. Tercero, J. Cernicharo, A. López, N. Brouillet, L. Kolesniková, | B. Tercero, J. Cernicharo, A. López, N. Brouillet, L. Kolesniková, | ||
reported on\\ | reported on\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
The authors used their IRAM 30 m line survey as well as ALMA Science Verfication data to claim a tentative detection of that molecule. The presented model looks promising, though some, possibly minor, issues are quite obvious. The ratio of dimethyl ether to ethyl methyl ether in their ground vibrational states of ≥ 150 appears reasonable, even if vibrational corrections will decrease the ratio considerably. In the absence of any other molecular features shown in the model, the detection should be viewed as tentative, as was done by the authors. | The authors used their IRAM 30 m line survey as well as ALMA Science Verfication data to claim a tentative detection of that molecule. The presented model looks promising, though some, possibly minor, issues are quite obvious. The ratio of dimethyl ether to ethyl methyl ether in their ground vibrational states of ≥ 150 appears reasonable, even if vibrational corrections will decrease the ratio considerably. In the absence of any other molecular features shown in the model, the detection should be viewed as tentative, as was done by the authors. | ||
+ | B. Tercero, S. Cuadrado, A. López, N. Brouillet, D. Despois, and J. Cernicharo\\ | ||
+ | investigated\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | They analyzed the Cycle 0 ALMA science verification data and found ethyl methyl ether beyond doubt. | ||
- | ---- | + | S. Manigand, J. K. Jørgensen, H. Calcutt, H. S. P. Müller, N. F. W. Ligterink, A. Coutens, M. N. Drozdovskaya, |
+ | reported on\\ | ||
+ | **[[https:// | ||
+ | //Astron. Astrophys.// | ||
+ | They found ethyl methyl ether toward IRAS 16293–2422 B in this context. | ||
- | Contributor(s): | ||
+ | ---- | ||
+ | |||
+ | Contributor(s): | ||
---- | ---- | ||