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| molecules:ism:glycol [2019/04/24 16:26] – mueller | molecules:ism:glycol [2019/10/24 09:53] (current) – mueller | ||
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| There is a report in the literature on detection of ethanediol, aka ethylene glycol, or briefly glycol, in Sgr B2(N-LMH): | There is a report in the literature on detection of ethanediol, aka ethylene glycol, or briefly glycol, in Sgr B2(N-LMH): | ||
| J. M. Hollis, F. J. Lovas, P. R. Jewell, and L. H. Coudert,\\ | J. M. Hollis, F. J. Lovas, P. R. Jewell, and L. H. Coudert,\\ | ||
| - | **[[http://dx.doi.org/ | + | **[[https:// |
| // | // | ||
| Because of the small number of lines and possible line overlap the detection should be viewed with some caution by itself. | Because of the small number of lines and possible line overlap the detection should be viewed with some caution by itself. | ||
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| More recently, two transition with complex velocity components have been detected in the centimeter range toward Sgr B2(N-LMH) employing the GBT:\\ | More recently, two transition with complex velocity components have been detected in the centimeter range toward Sgr B2(N-LMH) employing the GBT:\\ | ||
| J. M. Hollis,\\ | J. M. Hollis,\\ | ||
| - | **[[hollis_asilomar.pdf|Complex Molecules and the GBT: Is Isomerism the Key ?]]**,\\ | + | **{{ :pdfs:hollis_asilomar.pdf |Complex Molecules and the GBT: Is Isomerism the Key ?}}**, |
| Contribution at the IAU Symposium 231, Astrochemistry throughout the Universe, Asilomar, CA.\\ | Contribution at the IAU Symposium 231, Astrochemistry throughout the Universe, Asilomar, CA.\\ | ||
| While it is hard to say that the detection is beyond doubt, these two lines render the detection quite secure – mainly because the line density at these lower frequencies is fairly small. | While it is hard to say that the detection is beyond doubt, these two lines render the detection quite secure – mainly because the line density at these lower frequencies is fairly small. | ||
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| Contributor(s): | Contributor(s): | ||
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