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molecules:ism:etcn [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:etcn [2022/03/17 09:39] (current) – mueller | ||
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Ethyl cyanide, C< | Ethyl cyanide, C< | ||
D. R. Johnson, F. J. Lovas, C. A. Gottlieb, E. W. Gottlieb, M. M. Litvak, P. Thaddeus, and M. Guélin,\\ | D. R. Johnson, F. J. Lovas, C. A. Gottlieb, E. W. Gottlieb, M. M. Litvak, P. Thaddeus, and M. Guélin,\\ | ||
- | **[[http://cdsads.u-strasbg.fr/ | + | **[[https://ui.adsabs.harvard.edu/ |
- | // | + | // |
More recently, however, it has also been detected toward a low-mass star-forming region:\\ | More recently, however, it has also been detected toward a low-mass star-forming region:\\ | ||
S. Cazaux, A. G. G. M. Tielens, C. Ceccarelli, A. Castets, V. Wakelam, E. Caux, B. Parise, D. Teyssier,\\ | S. Cazaux, A. G. G. M. Tielens, C. Ceccarelli, A. Castets, V. Wakelam, E. Caux, B. Parise, D. Teyssier,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
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Ethyl cyanide in its two lowest vibrational states // | Ethyl cyanide in its two lowest vibrational states // | ||
E. Gibb, A. Nummelin, W. M. Irvine, D. C. B. Whittet, and P. Bergman,\\ | E. Gibb, A. Nummelin, W. M. Irvine, D. C. B. Whittet, and P. Bergman,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
This account apparently did not receive the appropriate attention. Later, observations toward Sgr B2(N-LMH) were reported:\\ | This account apparently did not receive the appropriate attention. Later, observations toward Sgr B2(N-LMH) were reported:\\ | ||
D. M. Mehringer, J. C. Pearson, J. Keene, and T. G. Philips,\\ | D. M. Mehringer, J. C. Pearson, J. Keene, and T. G. Philips,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
- | // | + | // |
These states as well as higher vibrational states up to v< | These states as well as higher vibrational states up to v< | ||
A. M. Daly, C. Bermúdez, A. López, B. Tercero, J. C. Pearson, N. Marcelino, J. L. Alonso, and J. Cernicharo, | A. M. Daly, C. Bermúdez, A. López, B. Tercero, J. C. Pearson, N. Marcelino, J. L. Alonso, and J. Cernicharo, | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
They were also detected in Sagittarius B2(N) by\\ | They were also detected in Sagittarius B2(N) by\\ | ||
A. Belloche, H. S. P. Müller, K. M. Menten, P. Schilke, and C. Comito:\\ | A. Belloche, H. S. P. Müller, K. M. Menten, P. Schilke, and C. Comito:\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
- | //Astron. Astrophys.// | + | //Astron. Astrophys.// |
The three < | The three < | ||
K. Demyk, H. Mäder, B. Tercero, J. Cernicharo, J. Demaison, L. Margulès, M. Wegner, S. Keipert, and M. Sheng,\\ | K. Demyk, H. Mäder, B. Tercero, J. Cernicharo, J. Demaison, L. Margulès, M. Wegner, S. Keipert, and M. Sheng,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
Laboratory Rotational Spectrum and Detection in Orion]]**\\ | Laboratory Rotational Spectrum and Detection in Orion]]**\\ | ||
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
They were also detected in Sagittarius B2(N) by\\ | They were also detected in Sagittarius B2(N) by\\ | ||
H. S. P. Müller, A. Belloche, K. M. Menten, C. Comito, and P. Schilke,\\ | H. S. P. Müller, A. Belloche, K. M. Menten, C. Comito, and P. Schilke,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
- | //J. Mol. Spectrosc.// | + | //J. Mol. Spectrosc.// |
The detection of the < | The detection of the < | ||
L. Margulès, R. Motiyenko, K. Demyk, B. Tercero, J. Cernicharo, M. Sheng, M. Weidmann, J. Gripp, H. Mäder, and J. Demaison,\\ | L. Margulès, R. Motiyenko, K. Demyk, B. Tercero, J. Cernicharo, M. Sheng, M. Weidmann, J. Gripp, H. Mäder, and J. Demaison,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
- | //Astron. Astrophys.// | + | //Astron. Astrophys.// |
The isotopolog was also detected in Sagittarius B2(N2), the northern, secondary hot-core of Sgr B2(N), by\\ | The isotopolog was also detected in Sagittarius B2(N2), the northern, secondary hot-core of Sgr B2(N), by\\ | ||
A. Belloche, H. S. P. Müller, R. T. Garrod, and K. M. Menten,\\ | A. Belloche, H. S. P. Müller, R. T. Garrod, and K. M. Menten,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
A. Belloche, H. S. P. Müller, R. T. Garrod, and K. M. Menten\\ | A. Belloche, H. S. P. Müller, R. T. Garrod, and K. M. Menten\\ | ||
were\\ | were\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
They report the tentative detection of deuterated ethyl cyanide in the course of their 3 mm line survey with ALMA. Their ratios of the normal species to the one deuterated at the out-of-plane methyl group position and at the methylene group are about 2000, the upper limit to the one deuterate at the in-plane methyl group position is 4000, consistent with the other positions which occur twice each. The number of clean lines was so small that the authors refrained from claiming a firm detection. | They report the tentative detection of deuterated ethyl cyanide in the course of their 3 mm line survey with ALMA. Their ratios of the normal species to the one deuterated at the out-of-plane methyl group position and at the methylene group are about 2000, the upper limit to the one deuterate at the in-plane methyl group position is 4000, consistent with the other positions which occur twice each. The number of clean lines was so small that the authors refrained from claiming a firm detection. | ||
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L. Margulès, A. Belloche, H. S. P. Müller, R. A. Motiyenko, J.-C. Guillemin, R. T. Garrod, and K. M. Menten,\\ | L. Margulès, A. Belloche, H. S. P. Müller, R. A. Motiyenko, J.-C. Guillemin, R. T. Garrod, and K. M. Menten,\\ | ||
reported on the\\ | reported on the\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
//Astron. Astrophys.// | //Astron. Astrophys.// | ||
The astronomical detection was made in Sagittarius B2(N2) in the course of their 3 mm line survey with ALMA. | The astronomical detection was made in Sagittarius B2(N2) in the course of their 3 mm line survey with ALMA. | ||
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Contributor(s): | Contributor(s): | ||
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