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molecules:ism:aceton [2019/02/25 22:38] – external edit 127.0.0.1 | molecules:ism:aceton [2019/04/24 16:19] – mueller | ||
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15 years later, this detection was confirmed: | 15 years later, this detection was confirmed: | ||
L. E. Snyder, F. J. Lovas, D. M. Mehringer, N. Y. Miao, Y.-J. Kuan, J. M. Hollis, and P. R. Jewell,\\ | L. E. Snyder, F. J. Lovas, D. M. Mehringer, N. Y. Miao, Y.-J. Kuan, J. M. Hollis, and P. R. Jewell,\\ | ||
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More recently, propanone was detected towards the high-mass star-forming region Orion KL: | More recently, propanone was detected towards the high-mass star-forming region Orion KL: | ||
D. N. Friedel, L. E. Snyder, A. J. Remijan, and B. E. Turner,\\ | D. N. Friedel, L. E. Snyder, A. J. Remijan, and B. E. Turner,\\ | ||
- | **[[http://dx.doi.org/ | + | **[[https:// |
// | // | ||
Besides a very large number of transitions in its ground vibrational state, a few lines of the first excited torsional state were reported. Even though the number of vibrationally excited lines is small, the consistent global modeling ensures this aspect of the detection. | Besides a very large number of transitions in its ground vibrational state, a few lines of the first excited torsional state were reported. Even though the number of vibrationally excited lines is small, the consistent global modeling ensures this aspect of the detection. | ||
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J. M. Lykke, A. Coutens, J. K. Jørgensen, M. H. D. van der Wiel, R. T. Garrod, H. S. P. Müller, P. Bjerkeli, T. L. Bourke, H. Calcutt, M. N. Drozdovskaya, | J. M. Lykke, A. Coutens, J. K. Jørgensen, M. H. D. van der Wiel, R. T. Garrod, H. S. P. Müller, P. Bjerkeli, T. L. Bourke, H. Calcutt, M. N. Drozdovskaya, | ||
reported on\\ | reported on\\ | ||
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This report is the first one on the detection of acetone around a low-mass protostar. The Protostellar Interferometric Line Survey (PILS) was carried out with ALMA in its Band 7 (329 – 363 GHz). A total of 186 lines were assigned to acetone. | This report is the first one on the detection of acetone around a low-mass protostar. The Protostellar Interferometric Line Survey (PILS) was carried out with ALMA in its Band 7 (329 – 363 GHz). A total of 186 lines were assigned to acetone. |